The galaxy presents as a single, relatively compact object. Its light profile appears smooth and centrally concentrated, displaying a gradual decrease in intensity from the core to the outer regions. The general shape is consistent with an elliptical morphology, with minimal evidence of spiral arms or a distinct disk structure. There may be slight irregularity in its shape, however, and its classification is somewhat uncertain.

The color profile shows a moderate gradient across the optical bands, with the core appearing slightly more yellow/red compared to the outer edges, which exhibit a somewhat bluer hue. This color difference could imply variations in the stellar populations, with older stars concentrated in the center. There does not appear to be a single distinct structure throughout.
