The galaxy presents an elliptical morphology. The central region exhibits a bright, concentrated core, suggestive of a high stellar density. A gradual decrease in luminosity is observed towards the outer regions. The galaxy appears relatively smooth in texture, with no discernible spiral arms or significant dust lanes visible in this image. The color profile indicates a higher concentration of older stellar populations, as evidenced by the yellowish-red hue of the core. There is little evidence of active star formation regions based on the limited blue color component. The overall form is mostly rounded, with only a slight elongation to the shape. There do not appear to be any signs of tidal disturbances or ongoing major mergers within the immediate vicinity of the galaxy.
