The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a generally smooth morphology with minimal discernible spiral arm structure. Its shape is closer to being in between round and cigar shaped. The light is concentrated towards the center, suggesting the presence of an older stellar population. The galaxy presents a yellow hue which might indicate the presence of older stars, it is relatively bright. There are no obvious signs of significant recent or ongoing major mergers or tidal disturbances, though some minor disturbance cannot be ruled out. The galaxy is likely a relatively massive system.
