The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a noticeable elongation, appearing cigar-shaped. The central bulge is prominent and has a yellowish hue, likely indicative of an older stellar population. The outer regions show a gradual decrease in luminosity without distinct spiral arm features. There is a subtle blue tint noticeable at the outer edges, perhaps signalling some recent, but limited, star formation. No significant signs of tidal disturbances or major mergers are visually apparent. Overall, the galaxy appears to be a passively evolving system.
