The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellowish hue, suggesting an older stellar population. Moving outward from the core, the galactic disk appears more diffuse, exhibiting a bluer tint. The overall shape is somewhat elongated, with the major axis being significantly larger than the minor axis. There is no apparent spiral arm structure, and the smoothness suggests a lack of recent major merging events. The galaxy's color indices indicate ongoing, but possibly low-level, star formation activity. There is a subtle asymmetry in the outer regions.
