The galaxy appears to be a relatively compact system, likely an early-type spiral or lenticular galaxy. Its overall shape is elliptical, with a noticeable, concentrated bulge towards the center. The light distribution is fairly smooth, indicating an older stellar population. There is a subtle hint of a disk component surrounding the bulge, but distinct spiral arms are not apparent, as the bulge overwhelms the overall structure. The galaxy exhibits a color gradient, with the central bulge appearing more yellow/red, suggesting a higher concentration of older, redder stars and dust. The outer regions have a faint hint of bluer light, which could indicate the presence of younger, hotter stars in the disc. There are no obvious signs of ongoing major mergers or strong tidal disturbances.
