The galaxy presents a generally smooth, elliptical morphology. It exhibits a noticeable central bulge characterized by a yellowish-white hue, suggesting an older stellar population. The light gradually fades from the center. Surrounding the core is a fainter, elongated disk-like structure exhibiting a bluer color, possibly indicative of ongoing, albeit moderate, star formation. The overall appearance is largely undisturbed, with no obvious signs of a major ongoing merger or tidal disruption. There is only a subtle asymmetry and some very slight irregularities on one edge of the galaxy.
