The galaxy appears to be a relatively smooth, elliptical system. Its central region exhibits a concentrated luminosity gradient, indicative of a prominent galactic nucleus. The overall color profile suggests a moderate population of older stars, contributing to a yellowish-white hue. There is little evidence of significant dust lanes or spiral arm structure. The galaxy shows some evidence of minor disturbances, potentially indicative of a past or ongoing minor merger event. It has a generally round shape, with a subtle elongation.
