The galaxy presents as a fairly regular elliptical shape, with a smooth light distribution, consistent with an early-type galaxy morphology. The color gradient suggests a more concentrated population of older stars toward the central region, which appears slightly yellow/white. There is no visual evidence of spiral arms or prominent dust lanes. The outer regions of the galaxy exhibit a bluer hue, which could suggest the presence of younger stellar populations, though this is subtle. The galaxy shows an elongated form, with an apparent axis ratio of approximately 0.65. No significant disturbances are visible.