The galaxy presents an overall smooth, elliptical morphology. The central region exhibits a bright, concentrated core, suggesting a significant stellar population density. Moving outwards from the center, the light gradually diminishes into a more diffuse halo. The galaxy's shape is elongated. There are no obvious signs of spiral arms or prominent dust lanes visible in this image. The color profile indicates a mixture of stellar populations, with a tendency towards older stars dominating the overall light. No apparent ongoing merger events or significant tidal disturbances are discernible. The galaxy appears relatively isolated and undisturbed.
