The galaxy presents as a generally smooth and centrally concentrated object. It exhibits a slightly elongated, possibly elliptical morphology, appearing more 'in between' round and cigar shaped. There is no strong indication of spiral arm structure or pronounced disk features visible in this image.

The color profile suggests a relatively evolved stellar population, with a yellow/orange hue dominating, possibly indicative of older stars. There is no evidence of a strong blue component suggesting minimal recent star formation. The galaxy does not appear to be undergoing any major merger activity.
