The galaxy presents as a somewhat elliptical, diffuse structure with a brighter, more concentrated central region. The core exhibits a reddish hue, suggesting a population of older stars or dust obscuration. Surrounding the central bulge, there is a more extended, fainter halo or disk-like component. This outer region appears less structured, with a mottled texture indicating some irregularity or ongoing star formation. Overall, the galaxy appears relatively smooth, with little evidence of strong spiral arms or a prominent bar. There is some asymmetry in the outer regions, which could indicate minor tidal interactions or disturbances.
