The galaxy presents as a largely smooth, elliptical object with a concentrated central bulge. The color profile indicates a relatively evolved stellar population, leaning toward a redder overall hue. There is a notable lack of distinct spiral arm structure or prominent dust lanes within the observable features. The galaxy exhibits a generally rounded morphology, showing no signs of major tidal disturbances or ongoing merger activity, with slight irregularities. The galaxy appears moderately luminous, suggesting a substantial stellar mass. The relatively smooth structure and color profile suggest it is a fairly mature system, possibly an early-type galaxy that is no longer actively forming stars at a high rate.
