The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in surface brightness towards its periphery. The color profile suggests a population of older stars, with a dominant yellowish-red hue in the central regions, possibly indicating a lack of significant ongoing star formation.  There is a fainter object to the side. This object appears similar to a star, it could be a star or globular cluster. There is no evidence of strong tidal features or significant morphological disturbances in the visible light, suggesting it is not currently undergoing a major merger.
