The galaxy appears to be a relatively luminous system, exhibiting a dominant central bulge with a high degree of radial concentration. The light profile suggests a smooth component, potentially an elliptical or S0 galaxy, though there are hints of a faint, disturbed disk surrounding the bulge. The galaxy is somewhat ellipsoidal, but trending to the more rounded end of the spectrum. The core region displays a yellowish tint, indicative of an older stellar population, while bluer regions are observed in the outer disk, suggestive of ongoing, albeit relatively mild, star formation. There is also evidence of a possible ongoing merger or interaction event, given a small amount of asymmetric light distribution and possible tidal features.
