The galaxy presents as a relatively smooth, centrally concentrated object. There is a slight elongation, but it is generally rounded. The color profile suggests a population dominated by older stars, with a redder central region and slightly bluer peripheries indicating some ongoing star formation. There is evidence of a minor disturbance in its morphology, suggesting a possible interaction or recent minor merger. The galaxy shows no prominent spiral arm structure or a strong bar. It is a likely candidate for an early-type galaxy or a late-type galaxy with a large bulge.
