The galaxy presents with an elliptical morphology, exhibiting a smooth, centrally concentrated luminosity profile. The core region shows a distinct yellowish-white color, suggestive of an older stellar population likely dominated by red giant stars. Moving outward from the center, the galaxy gradually fades into a less defined, slightly elongated halo with hints of a blueish color. The overall structure is largely undisturbed, with only subtle indications of minor disturbances possibly from a past interaction or merger. No strong spiral arm features or prominent dust lanes are visible. The isophotes appear relatively regular and symmetrical, although there are some subtle irregularities in the outer regions. Based on these characteristics, the galaxy is consistent with an early-type galaxy, potentially an elliptical or lenticular galaxy at significant distance.
