The galaxy presents a generally smooth morphology, appearing elliptical or lenticular in shape. There is a concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. The surrounding disk or halo exhibits a bluer tint, possibly indicating the presence of younger stars or ongoing star formation, though the smoothness suggests the star formation rate is low to moderate. The galaxy appears mostly undisturbed, with no obvious signs of major mergers or tidal interactions. It presents as a relatively isolated galaxy.
