This galaxy exhibits a predominantly smooth morphology. The central bulge appears bright and concentrated, with a yellowish hue, suggestive of an older stellar population. There is a slight elongation to the galaxy's shape, moving it away from being perfectly round, but not appearing as a highly elongated or cigar-shaped system. Faint disk-like features are subtle. The overall color profile indicates that this is most likely an elliptical or lenticular galaxy. There's no clear evidence of major ongoing mergers or significant tidal disturbances in the immediate vicinity, though a very slight, minor asymmetry to the extended outer regions might be present. The galaxy is relatively isolated.
