The galaxy presents as an elliptical morphology, elongated with a cigar-shaped appearance. The central bulge exhibits a smooth, concentrated light profile, suggesting a high stellar density and an older stellar population. The light is yellowish-white, consistent with evolved stars and a relatively low rate of star formation. There is no distinct spiral arm structure or prominent dust lane visible. The overall impression is that of a relatively quiescent galaxy, likely a late-type elliptical or an S0 galaxy seen at an angle. There are no obvious signs of major mergers or tidal disturbances.
