The galaxy presents a generally elliptical morphology, displaying a central bulge that appears relatively smooth and concentrated. The core exhibits a yellowish hue, potentially indicative of an older stellar population. Fainter, bluer regions extend outwards from the central bulge, these may trace faint spiral arm structures. The overall smoothness and lack of prominent spiral arms suggests it is potentially an early-type spiral galaxy. There is no obvious evidence of strong ongoing star formation, the colors point towards a later type galaxy with an older population of stars. The lack of any strong tidal features suggests this galaxy does not have any major mergers occurring. The galaxy's shape appears more elongated than circular.
