The galaxy exhibits an elliptical morphology, with a smooth, centrally concentrated luminosity profile. The core region presents a yellowish-white hue, indicating an older stellar population likely dominating this area. The isophotes are roughly elliptical, with a minor axis to major axis ratio of approximately 0.8, suggesting a modest degree of flattening. The galaxy lacks any obvious spiral arm structures or prominent dust lanes. The outer regions exhibit a gradual decrease in surface brightness, transitioning to a bluer color suggestive of younger stars. There are no apparent signs of recent major merger activity or significant tidal disturbances. The galaxy appears to be relatively isolated with no close interacting companions visible in the immediate vicinity.
