This galaxy exhibits a generally smooth morphology, appearing as an elliptical structure. The central region presents a concentrated and brighter luminosity, suggestive of a dense stellar population or potentially an active galactic nucleus. The color gradient indicates a population of older stars, particularly towards the central bulge, contributing to the yellowish hue. Faint hints of bluer regions at the edge of the galaxy suggest some degree of ongoing star formation. There are no obvious signs of tidal disturbances or merging activity based on this observation. The galaxy's overall shape appears relatively undisturbed and relaxed.
