The galaxy presents a relatively smooth, elliptical morphology with an overall golden hue, indicative of an older stellar population. The core exhibits a bright, concentrated luminosity profile, suggesting a high stellar density in the central region. Moving outward from the core, the luminosity gradually decreases. There is minimal indication of spiral arm structure or significant dust lanes. The shape deviates slightly from perfectly circular, displaying a mild elongation. Subtle disturbances are possibly present in the outer regions, though this requires further investigation with higher resolution imaging. Based on the overall color and smooth appearance, this galaxy is potentially an early-type galaxy at a moderate redshift.
