The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, which dominates its overall light profile. There appears to be a minimal disk component, and no discernible spiral arms. Its color is primarily yellow-red, which suggests an older stellar population with a lower rate of on-going star formation. There is no evidence of any major mergers or significant tidal disturbances, though a minor disturbance may be possible. The galaxy appears to be roughly circular in shape.
