The galaxy presents as a moderately luminous system, appearing largely smooth in texture. A dominant central bulge region is evident, exhibiting a bright, concentrated core. Fainter, diffuse light extends outwards from the core, suggesting the presence of a surrounding galactic disk. The overall morphology appears somewhat disturbed, potentially indicative of a previous or ongoing interaction. Asymmetry is present in the outer regions. There appear to be multiple objects in close proximity, one presenting with a reddish hue, that could be indicative of a larger merger. The roundness indicates an elliptical morphology, but the extended nature of the outer disk could mean it has spiral features. The galaxy has an estimated mass consistent with that of a large galaxy, and the moderate star formation rate suggests it is undergoing active stellar production.
