This galaxy presents as a largely featureless, elliptical-like object. The central region is substantially brighter than the surrounding halo, showing a strong concentration of light and stellar density towards the core. The galaxy appears generally round with no distinct spiral arm structures, indicating a relatively smooth distribution of stars. The outer regions of the galaxy fade gradually into the background, suggesting a diffuse halo of stars. Color-wise, the galaxy displays a yellowish hue, hinting at a population of older stars. There are no signs of major tidal disturbances or ongoing mergers; however, there is a slight asymmetry to the shape and some very subtle color variations that could indicate a minor interaction or internal activity. Overall, the galaxy seems to be a relatively evolved system.
