The galaxy appears as a single, concentrated luminous object. Its overall shape appears relatively round, lacking any obvious spiral arms or bar-like structures. There is a bright, well-defined core, suggesting a high concentration of stars and possibly a supermassive black hole actively accreting material at the center. The galaxy exhibits a smooth, diffuse halo extending outwards from the bright core. The outer regions fade gradually, indicating a decreasing density of stars. The color is generally bluish in the central region, shifting towards reddish hues in the outer halo. This color gradient may reflect differences in stellar populations, with the central region containing younger, bluer stars, while the outer halo contains older, redder stars. There is no evidence of significant dust lanes or other obscuring material within the galaxy. The overall morphology suggests that this is likely an elliptical or lenticular galaxy, with a substantial spheroidal component. Based on the color profile and lack of distinct features, the galaxy is likely undergoing moderate star formation. There is no clear evidence of tidal disturbances or recent interactions with other galaxies.
