The galaxy appears to be a relatively smooth, elliptical system. Its central region is luminous, with a concentrated core that seems to diminish gradually. The overall shape is somewhat round, with a slight elongation that is neither extremely flattened nor cigar-shaped. There is no apparent structure of spiral arms or a distinct disk. There is no indication of tidal tails, merging features, or significant morphological disturbances that would suggest a major interaction. The light emitted is bluer in the central region, which may indicate star formation or the presence of hotter stars.
