The galaxy presents as a luminous elliptical system, characterized by a smooth, centrally concentrated light distribution. The overall color profile suggests a population of older stars, as the galaxy appears redder, with very little evidence of blue star formation regions. The galaxy exhibits a notable ellipticity and is somewhat elongated in shape. There is no evidence of a prominent disk structure or spiral arms, indicating a lack of significant ongoing star formation. The light distribution appears relatively undisturbed, with no major morphological disruptions or tidal features readily apparent, suggesting that the galaxy has not undergone a recent major merger event. There are several nearby galaxies, but none of them appear to be severely distorting the shape of this galaxy. 
