The galaxy presents as a primarily smooth, centrally concentrated object. Its overall shape is close to round, with a minor axis to major axis ratio approaching unity. There's an apparent lack of significant spiral structure or a distinct disk component upon visual inspection. Color gradients across the galaxy's body show a slight reddening towards the center, suggestive of an older stellar population concentrated in the core. The outer regions exhibit a bluer hue, potentially indicating younger stars or ongoing, albeit low-level, star formation. There is no visual evidence of major mergers or tidal disturbances in the immediate vicinity. The galaxy is fairly compact and luminous, showing a somewhat high mass estimate, and potentially quiescent with relatively low ongoing star formation activity, most prominently in the central region.