The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. There is little evidence of spiral arms or a significant disk structure. The galaxy exhibits a somewhat spheroidal morphology, leaning towards a round shape. No strong tidal features or signs of a major merger event are immediately apparent, although there might be subtle disturbances present. The color profile indicates a population of older stars, with a reddish hue dominating the central regions. The star formation rate appears to be relatively low.
