The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, which transitions outwards into a fainter, more diffuse halo. The color appears generally redder, indicative of an older stellar population and reduced ongoing star formation activity. There is no obvious spiral structure. The object is fairly compact, and the light profile is relatively smooth with hints of asymmetries, possibly suggesting it has experienced a minor disturbance from some interaction. Overall, this galaxy appears to be relatively evolved and quiescent.
