The galaxy presents as a centrally concentrated elliptical system, exhibiting a smooth, spheroidal morphology. It is elongated, appearing more cigar-shaped than circular. The core region is significantly brighter and exhibits a yellowish hue, indicative of an older stellar population. The galaxy lacks any obvious spiral arm structure or prominent dust lanes. There appears to be some faint, diffuse structure extending from the main body of the galaxy, perhaps tidal debris. There is no strong indication of a major ongoing merger event, but a small disturbance may exist within the galaxy.
