This galaxy appears to be a relatively smooth, elliptical-like system, exhibiting a concentrated central bulge. The galaxy displays a yellowish hue, suggesting an older stellar population. It is mostly smooth in appearance with some evidence of a possible tidal tail or minor disturbance extending from one end. It does not appear to be actively undergoing a major merger, but may have experienced a merger event in the past, given its structure. The galaxy is moderately luminous.
