The galaxy presents as a somewhat smooth, centrally concentrated object. The core exhibits a yellowish hue, suggesting a population of older stars. A gradual decrease in surface brightness is observed moving outward from the center, transitioning from a yellowish to a bluish-white color. This suggests the presence of a younger stellar population within the galaxy's outer regions, but it remains subtle. The overall shape appears largely elliptical, approaching circular. There are no clearly visible spiral arms or bar structures. There is a slight asymmetry, possibly indicating a minor gravitational disturbance or interaction. Evidence for recent or ongoing major mergers is absent. Based on the color profile, the galaxy is experiencing some degree of star formation.
