The galaxy presents as an elliptical-like form with a moderately smooth texture. The primary structure exhibits a pronounced central bulge, characterized by a concentration of older stars, indicated by its yellowish hue.  A faint, flattened disk-like structure is observed extending outwards from the bulge; this is indicative of more recent star formation activity due to its orange tint. The overall shape is an ellipse, but leans to a slightly more cigar-shaped form. No strong signs of tidal disturbances or ongoing mergers are visually apparent.  The star formation rate appears subdued overall, typical of older galaxies, though a subtle disk indicates more recent activity.
