The galaxy presents a moderately inclined, disk-like structure. Its overall appearance is relatively smooth. A bright central bulge dominates the luminosity profile. There is an extended halo of diffuse light. Faint reddish regions can be observed along the outer edges of the disk, which could signify areas of ongoing or recent star formation. The galaxy appears to be slightly elongated. There is no clear indication of strong tidal disturbances or major ongoing mergers.
