The galaxy presents a generally smooth morphology, although there is some evidence of more complex features that might represent a disk component. The galaxy appears centrally concentrated, with a bright, yellowish core indicating a concentration of older stars. The outer regions exhibit a bluer hue, suggesting the presence of some younger stellar populations. The overall shape is somewhat elliptical but deviates significantly from a perfect ellipse. It is difficult to say whether this is due to tidal disturbance or internal structure. There is no strong visual indication of a major ongoing merger, although subtle asymmetries are present that could be indicative of minor interactions. There is little to no evidence of strong star formation.
