This galaxy appears to be a relatively compact object with a smooth, elliptical morphology. The central region exhibits a bright, concentrated core that suggests a high stellar density. The overall color profile indicates a population of older stars, likely with low ongoing star formation. There are possibly merging companions involved in the galaxy's evolution, which could explain the disturbances observed in the main galaxy's structure. There are at least 2 other objects that appear to be in proximity to the main galaxy, and the objects appear to have undergone some tidal distortion. The color of these objects suggest a redder population of stars, potentially due to an older stellar population. The galaxy itself does not show strong evidence of a distinct disk structure and lacks prominent spiral arms.
