The galaxy presents as a centrally concentrated, smooth object, elliptical in shape. Its core exhibits a noticeable yellowish-red hue, suggesting a population of older stars. A faint, somewhat amorphous extension is observed to the right side of the core, appearing less defined and bluer in color, possibly indicating some level of ongoing or recent star formation activity. The overall symmetry points towards a system that is not strongly undergoing major disruptive processes such as a major merger, although the extension suggests a possible interaction or minor disturbance.
