The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright core that fades gradually outward. The color profile is suggestive of an older stellar population, with a dominant yellowish-red hue. There is an indication of a possible minor disturbance or companion object in proximity to the primary galaxy. This secondary object appears fainter and smaller, potentially interacting or in the process of merging with the larger galaxy. No distinct spiral arms or features associated with active star formation are clearly visible.
