The galaxy presents as a single, fairly compact object with a generally elliptical morphology. There is a noticeable color gradient, with a concentration of bluer light appearing more concentrated on one edge/side, suggesting potential ongoing star formation activity in that region. The bulk of the galaxy displays a yellowish-orange hue, likely indicative of an older stellar population and lower rates of star formation. The overall light distribution seems relatively smooth. The lack of strong spiral arm structures or obvious tidal features suggests this galaxy has likely undergone significant dynamical relaxation. There is a minor indication of disturbances or interactions, with the aforementioned bluer part appearing as a discrete clump.
