The galaxy presents a relatively smooth, centrally concentrated luminosity profile. There is a faint, disk-like structure present, but the overall morphology is dominated by a central bulge. The primary light emitted from the galaxy appears to be a cyan hue, suggesting a stellar population with ongoing or recent star formation. The system lacks any visually obvious strong spiral arm features or prominent dust lanes. No significant tidal disturbances or morphological indications of recent major merger events are apparent, however a potential small merger could be occurring. The shape of the galaxy is approximately round, with a slight tendency toward being in between round and elongated. The diameter of the galaxy appears to be approximately 6 kpc.
