The galaxy presents a moderately smooth, elongated profile, suggestive of an elliptical morphology, though a faint disk cannot be completely ruled out. There is a centrally concentrated bright region that diminishes in intensity with radial distance. The overall color appears relatively uniform, with a slightly bluer hue. No distinct spiral arms or significant dust lanes are readily apparent. The galaxy appears relatively isolated, showing no signs of significant tidal distortion or ongoing major merger activity, although the presence of a minor disturbance cannot be excluded. The relatively smooth appearance indicates a lack of significant current star formation, which suggests that it is a more evolved galaxy.
