The galaxy appears as a slightly elongated, lenticular or early-type spiral system. A smooth, centrally concentrated bulge dominates the light profile, exhibiting a yellowish hue suggestive of an older stellar population. Fainter, diffuse, bluer regions are present along the apparent minor axis extending from the main body of the galaxy; these may be hints of spiral arms, or tidal streams. There is no obvious dust lane visible across the galaxy's disk. The overall morphology suggests the galaxy is in a relatively evolved state, with a subdued star formation rate. The elongated shape indicates a possible recent interaction or a more inherent triaxial nature to the galaxy's structure.
