The galaxy presents a generally smooth, elliptical morphology. The central bulge region appears bright and concentrated, exhibiting a yellowish hue, which could suggest an older stellar population. There is a gradual decline in luminosity moving outwards from the core. The surrounding halo appears less defined, with a fainter, bluer color, possibly indicative of some ongoing star formation. Faint, diffuse reddish areas are scattered throughout, which might be regions of dust or HII emission. The galaxy is relatively undisturbed, lacking any obvious signs of major merger activity, although there may be some minor tidal features suggesting past interactions. The overall shape is approximately round, with only a slight elongation.
