The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely round with a subtle deviation towards a slightly elongated shape. The core region displays a bright, concentrated luminosity, suggesting a high stellar density and/or active galactic nucleus. The galaxy's color profile indicates a prevalence of older stellar populations. The disk may be almost entirely composed of older stars or there may be dust obscuring it. There's no obvious evidence of spiral arm structure or significant dust lanes. No indications of ongoing major merger events or tidal disturbances are apparent, but minor disturbances can not be ruled out. Overall, it appears to be a mature, relatively quiescent galaxy.
