The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a centrally concentrated light profile. The core region is characterized by a bright, yellowish hue, suggestive of an older stellar population. Moving outward from the core, the color transitions slightly toward redder tones, with a subtle indication of a disk-like component that is difficult to distinguish. There are no obvious spiral arm structures or signs of significant dust lanes. There appears to be minimal evidence of ongoing major mergers or tidal disturbances; the overall morphology suggests a system that has undergone significant dynamical relaxation. The roundness and smooth appearance point towards it being a potential elliptical galaxy. The galaxy displays a moderate redshift, indicating a substantial distance. This galaxy is of significant mass and low star formation.
