The galaxy presents as an elliptical morphology, with a generally smooth appearance and a high degree of central concentration. The color profile suggests a population of older stars, with the central bulge appearing more yellow/gold. There is some evidence of bluer components within the overall structure, suggesting a small amount of ongoing or recent star formation. The light distribution exhibits an elliptical shape, with a slight elongation visible. There are no discernible spiral arms, bars, or other prominent features typically associated with disk galaxies. There might be minor disturbances to the shape of the main galaxy body, but no major mergers or significant tidal features are visible. The overall appearance is consistent with a galaxy that has largely ceased active star formation.
