The galaxy presents a generally smooth morphology, appearing as an elliptical or lenticular type system. The central region displays a concentration of light, suggesting a significant stellar population or active galactic nucleus. A discernible color gradient is observed, with the core exhibiting a yellowish hue, potentially indicative of older stellar populations. The outer regions transition towards a bluer color, suggestive of younger, hotter stars or ongoing star formation, albeit at a low rate. The galaxy's shape is moderately elongated. There is no obvious indication of spiral arms, bars, or a significant dust lane within this image. Minor disturbances or tidal features are not readily apparent. The overall structure appears relatively undisturbed, characteristic of a galaxy that has likely undergone significant evolutionary processing.
