The galaxy exhibits a predominantly smooth morphology. The light distribution is centrally concentrated, appearing brightest towards the core. There is a notable lack of distinct spiral arm structure or prominent dust lanes. The overall shape seems to be somewhat elliptical, though not perfectly circular. The color profile indicates a redder core region, transitioning to slightly bluer hues in the outer regions, suggesting a mix of older stellar populations centrally and possibly some younger stars in the periphery. There appears to be no significant evidence of ongoing major merger activity or strong tidal disturbances, though subtle signs of a minor disturbance cannot be ruled out. The galaxy does not show any pronounced bar structure. The outer edges of the galaxy gradually fade into the background, indicative of a diffuse halo component.
