The galaxy presents as a luminous, elliptical structure. It is characterized by a smooth, centrally concentrated light distribution, with a gradual decrease in luminosity extending outwards. The core region exhibits a yellowish-orange hue, suggestive of an older stellar population. The galaxy lacks any visually discernible spiral arms or dust lanes. The overall morphology is elongated, appearing cigar-shaped, though with somewhat rounded edges. There is no obvious evidence of ongoing major mergers or significant tidal disturbances. There might be a minor asymmetry to the outer halo. Based on the observed color and morphology, this galaxy is most likely a massive elliptical galaxy with a relatively quiescent star formation rate.
