The galaxy presents as a fairly smooth, elliptical-like structure. The central region exhibits a concentrated, bright core with a reddish hue, potentially indicating an older stellar population. This central bulge transitions into a surrounding disk or halo. The halo region appears bluer than the core suggesting more recent star formation. The overall shape appears somewhat flattened, but not to the extent of a spiral galaxy. There is no clear evidence of a major ongoing merger or tidal disruption, although some minor irregularities in the outer regions are not ruled out based on this image.
