The galaxy presents as a generally elliptical, early-type system with a smooth, featureless morphology. The core region exhibits high luminosity, concentrated toward the center, indicating a significant population of older stars. The color gradient transitions from a yellowish-white core to a slightly bluer hue in the outer regions, suggesting a moderate level of on-going star formation despite the dominant older stellar population. There are no apparent spiral arms or prominent dust lanes visible in the image. The galaxy appears relatively isolated with no clear signs of major mergers, though there might be slight asymmetrical features.