The galaxy appears as a relatively smooth, elliptical-shaped object with a concentrated central bulge. The color profile suggests an older stellar population, exhibiting a yellowish-red hue. There is little evidence of prominent spiral arms or significant dust lanes. The light distribution seems to follow a centrally concentrated profile, with a gradual decrease in brightness from the core outwards. There might be a slight asymmetry in the outer isophotes, suggesting a possible interaction or minor disturbance, however, the bulk of the galaxy appears undisturbed.
