The galaxy presents as a fairly smooth, elliptical object with a slight elongation. It is likely an early-type galaxy. There is a faint, diffuse halo surrounding the central region. The core appears to be more luminous with a distinct, concentrated region. There is no apparent spiral structure or dust lanes. No significant tidal features or distortions are visible, suggesting it is not currently undergoing a major merger. The overall color indicates that it is likely comprised of an older stellar population, with very little ongoing star formation. The galaxy's shape is generally classified as in between round and cigar shaped, with a slight preference to round. No merger is currently ongoing. 
