The galaxy presents a smooth, somewhat elliptical morphology. There is little to no visible disk structure or prominent spiral arms, suggesting a later-type classification. The galaxy exhibits a moderate concentration of light towards the center, indicating the presence of a central bulge or core. The overall color appears relatively red, hinting at an older stellar population with lower ongoing star formation. No signs of significant mergers or tidal disturbances are immediately apparent, suggesting the galaxy is relatively undisturbed. There is a slight elongation or flattening of the galactic shape, but it does not appear cigar shaped. The galaxy appears to be isolated, with no other major galaxies in close proximity.
