This galaxy exhibits a predominantly smooth morphology, suggesting an elliptical or lenticular type. It has a slightly elongated shape, deviating from perfectly spherical. The central region displays a brighter, more concentrated luminosity, indicative of a bulge. A faint, diffuse disk may be present, but any spiral arm structures are not discernible. The galaxy appears to be in a relatively quiescent state, with no major mergers or significant tidal disturbances evident. A slight color gradient is observed, with the central bulge showing a yellower hue compared to the outer regions, which exhibit a somewhat bluer tint. This color difference may suggest older stellar populations dominating the bulge and comparatively younger populations populating the disk if it exists.
