The galaxy presents as a relatively smooth, elliptical-like object. Its overall color appears to be slightly yellow or golden, suggesting a population of older stars and/or significant dust content. The light distribution is concentrated towards the center, with a noticeable drop-off in surface brightness towards the edges. The galaxy's shape appears nearly round, exhibiting minimal elongation or discernible disk features. There are no prominent signs of spiral arms or any substantial irregularities that would indicate a recent or ongoing major merger event. There might be a very faint hint of a disturbance to the top side of the galaxy, as there is some slight visual disruption in the symmetry. This feature appears subdued, suggesting a potential minor interaction or internal dynamical process. Overall, the galaxy's morphology suggests a system undergoing relatively quiescent evolution.
