The galaxy appears to be a relatively smooth elliptical, potentially of type E3-E5, exhibiting a notable degree of ellipticity. It presents a concentrated central bulge, which gradually fades into a more diffuse halo. There seems to be a slight color gradient across the galaxy, with the central regions appearing somewhat redder than the outer parts, possibly indicating an older stellar population towards the center. There's little evidence of spiral arm structure or prominent dust lanes. The object is relatively compact, with a defined edge. Based on visual inspection, it appears to be a mature galaxy with limited ongoing star formation. Faint tidal features are possibly present, but not clear. The galaxy's overall appearance suggests it is a relatively isolated system, not currently undergoing a major merger.
