The galaxy appears to be a relatively smooth, elliptical or lenticular system. There is evidence of a centrally concentrated bulge that transitions smoothly into a broader, less defined disk-like structure. The color gradient indicates a population of older stars in the central region, appearing more yellow and red. The disk exhibits a bluer hue, suggesting the presence of some ongoing star formation, although the overall star formation rate appears to be relatively low. The galaxy exhibits a slightly elongated shape and does not appear to be undergoing any major merging events or showing significant tidal disturbances.
