The galaxy appears to be a relatively smooth, lenticular type, exhibiting a flattened, disk-like structure. Its color profile is dominated by blue hues, suggestive of a younger stellar population and ongoing, though subdued, star formation. The galaxy's light is fairly evenly distributed, with no pronounced spiral arms or bar features evident. There is a slight elongation, indicating a shape somewhere between perfectly round and cigar-shaped. Faint hints of disturbances and asymmetrical features suggest the possibility of minor gravitational interactions or past mergers.
