The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. It exhibits a yellowish hue, suggestive of an older stellar population, with diminished rates of current star formation. The shape is moderately elongated, neither perfectly spherical nor extremely flattened. There is no apparent evidence of ongoing major mergers or tidal disturbances, although subtle minor irregularities cannot be ruled out based on visual inspection alone. The overall structure is consistent with that of an early-type galaxy, likely a lenticular or elliptical galaxy at a moderate redshift.
