The galaxy exhibits a generally smooth, elliptical morphology, appearing largely featureless upon visual inspection. The core region is characterized by a bright, concentrated luminosity, suggesting a high stellar density and potentially the presence of an active galactic nucleus or supermassive black hole. Moving outward from the core, the luminosity gradually decreases, transitioning into a more diffuse halo. The galaxy displays a slightly elongated, though largely round, shape with a minor axis that is only a little smaller than the major axis. There is a very faint and diffuse asymmetry on one side of the galactic disk. This galaxy appears to be in a relatively quiescent state, without evidence of significant ongoing star formation from the image alone. There are no signs of major disturbances or mergers. The overall color profile indicates a mature stellar population. The relatively redder hue in the central region suggests an older population of stars.
