The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution appears concentrated towards the center, suggesting a prominent bulge. There is a discernible color gradient, with the central region exhibiting a yellower hue, possibly indicative of an older stellar population. Fainter, bluer extensions are tentatively observed further out from the central bulge. The galaxy does not appear to display any obvious signs of strong tidal interactions or ongoing major merger activity. Some asymmetry is present in the outer regions, possibly due to a minor interaction. There are hints of a faint disk-like structure or spiral arms.
