The galaxy presents as a relatively smooth object, exhibiting a generally elliptical morphology. Its shape is elongated. The central region displays a brighter, more concentrated luminosity, suggestive of a bulge or nucleus. Proceeding outward from the center, the luminosity gradually diminishes, with no clear evidence of spiral arm structures. There appear to be a population of older stars at the center. It is likely a massive galaxy with a relatively low star formation rate. There might be signs of minor disturbances.
