The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated light profile, with a bright, compact core. The galaxy's overall shape is close to circular, lacking any significant elongation or asymmetry. There is some evidence of a faint, diffuse halo surrounding the central region, which is approximately 4 kiloparsecs in radius. The primary color of the galaxy appears to be a combination of yellow and white, with subtle hints of blue around the core. This color suggests an older stellar population. There is no strong indication of spiral arm structure or significant dust lanes, implying a lack of ongoing major star formation. The observed morphology is consistent with a galaxy that is not undergoing a major merger. Small disturbances may be present around the disk.
