The galaxy exhibits a roughly elliptical morphology with a bright, relatively compact core. A fainter, more diffuse region surrounds the core. The core is primarily bluish-green, suggesting the presence of younger, hotter stars or strong emission lines. The outer regions display a reddish hue, potentially indicating older stellar populations or dust extinction. There is a subtle distortion or irregularity in the shape of the outer regions, potentially hinting at a minor gravitational interaction or disturbance. There may be some weak evidence of a very subtle disk-like component, although this is not clearly defined. Overall, the galaxy appears to be an intermediate system, displaying characteristics of both elliptical and spiral galaxies, and possibly undergoing some form of interaction.
