The galaxy presents a generally smooth, elliptical morphology. It is characterized by a centrally concentrated bulge region exhibiting a yellowish hue, possibly indicative of an older stellar population. The light profile appears to gradually fade outwards from the core. There may be a slight disk-like structure present; however, this is only barely perceptible due to its small size. No spiral arms are apparent, and there does not appear to be any signs of a major ongoing merger. Overall, this galaxy is fairly massive with an absence of substantial star formation.
