The galaxy presents as a moderately luminous, elongated system. A bright central bulge dominates the galaxy's core, with an apparent flattening and ellipticity extending outwards. The bulge appears to have a smooth profile. The overall colour suggests a combination of evolved stellar populations and ongoing star formation. The galaxy does not present clear signs of spiral arm structures or strong tidal disturbances. The relative smoothness and colour characteristics suggest a disk galaxy. The distribution of light indicates that the older stellar population is concentrated towards the center.
