The galaxy presents as a flattened ellipsoid, suggestive of a disk galaxy observed at an oblique angle. Its light is dominated by a bright central bulge. This bulge appears relatively smooth and unresolved, likely consisting of an older stellar population.

Surrounding the bulge is a fainter, more diffuse disk. The disk exhibits a subtle blue tint, indicating the presence of some younger stars, however the star formation rate appears relatively low. There is some slight asymmetry in the disk, possibly indicating a minor gravitational disturbance or recent interaction. There is no clear evidence of spiral arm structure.

The galaxy shows no obvious signs of a major ongoing merger or significant tidal disruption. Its overall morphology is indicative of a relatively quiescent galaxy with moderate mass.
