The galaxy presents as a centrally concentrated object, exhibiting a smooth, generally elliptical morphology. The core region displays a high degree of luminosity, characterized by a yellow-white hue indicative of an older stellar population. The light diffuses outward, transitioning to a more indistinct, fainter halo. This outer region exhibits lower surface brightness, yet still maintains a largely smooth appearance. Some faint irregularities and slight extensions are apparent, which might be tidal debris or a minor interaction. The galaxy shows no pronounced spiral arm structure or significant dust lane features, pointing to a morphology tending towards an elliptical classification. The relatively round shape suggests it is not strongly flattened. There are no clear indications of ongoing major mergers, although subtle perturbations suggest potential minor disturbances. Overall, the galaxy appears to be a relatively evolved system dominated by older stellar populations, with signs of potential past or ongoing minor interactions.
