The galaxy presents as a relatively smooth, elliptical-like structure with a noticeable central bulge. The light distribution appears concentrated towards the center, fading gradually towards the outer edges. The galaxy exhibits a slightly elongated shape with a primary axis running approximately diagonally across the image. The overall color profile suggests a population of older stars, though there may be evidence of some ongoing star formation, hinted at by the subtle bluish tones particularly in the outer regions. There do not appear to be any major disturbances or tidal features indicative of recent major mergers, but the disk does appear slightly disturbed which may be due to a minor merger.
