This galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, with a subtle elongation evident. The galaxy exhibits a color gradient, appearing more yellow-white towards the core, suggestive of an older stellar population dominating the central regions. Fainter, slightly bluer hues are observed towards the outer regions, potentially indicating the presence of some younger stars or ongoing, albeit low, star formation. No distinct spiral arms or bar structures are discernible. There is a slight asymmetry with a possible disturbance indicating an ongoing or past minor merger event. The overall morphology suggests a relatively massive galaxy, likely an early-type system, with a relatively inactive star formation rate for its mass.
