The galaxy appears to be an elliptical galaxy, characterized by a smooth, concentrated luminosity profile. Its morphology is largely featureless, lacking any readily discernible spiral arms or prominent dust lanes. The overall shape approximates a sphere, with minimal elongation. There is a high degree of central concentration, indicated by the bright, relatively compact core. A diffuse halo of light extends outward from the core, gradually fading into the background sky. There is no indication of ongoing major merger activity or significant tidal disturbances affecting the galaxy’s structure, although some very minor irregularity cannot be ruled out based on this image alone. The galaxy exhibits a color gradient, appearing slightly bluer in the central regions, suggestive of recent or current star formation, and gradually becoming redder in the outer regions. The galaxy is of moderate size and luminosity.
