The galaxy presents as a luminous, centrally concentrated object, exhibiting a somewhat smooth morphology. It appears moderately elliptical in shape, with an approximate major axis of roughly 6 Kpc. The galaxy's light profile suggests a dominant bulge component. A minor, reddish secondary light source is detected to the right of the primary galaxy core, which may indicate a region of active star formation or a smaller interacting dwarf galaxy. The overall color index indicates the galaxy is likely a relatively evolved system, although some ongoing star formation cannot be excluded. There is no obvious evidence of strong tidal features or major morphological disturbances.
