The galaxy presents as an elongated, lenticular or possibly elliptical structure with a smooth light distribution, displaying a significant axis ratio. The object is characterized by a central concentration of light, which appears yellow-white, indicative of a population of older stars. This suggests a relatively quiescent star formation history. The absence of clear spiral arm structures or prominent dust lanes supports the hypothesis of an early-type morphology. The outer regions exhibit a faint, diffuse halo. There is no visible evidence of ongoing major mergers or tidal disturbances affecting its structure, though the lack of high-resolution imaging limits our ability to detect faint tidal features. The galaxy exhibits a redshift suggesting a considerable distance. Based on the colors, mass, and star formation estimates, this galaxy appears to be relatively massive with a low star formation rate.
