The galaxy appears as a bright, centrally concentrated object, likely an elliptical or lenticular galaxy. It exhibits a generally smooth, rounded morphology, with a gradual decrease in luminosity from the core outwards. The core region presents a yellowish hue, potentially indicating a population of older stars. Faint disk-like structure may be present, based on a possible asymmetry. The absence of prominent spiral arms or significant dust lanes points away from a spiral classification. No strong evidence of ongoing major merging events, but some minor disturbances cannot be ruled out. The overall color profile suggests a relatively low rate of star formation within the galaxy at its current epoch.
