This galaxy presents as a generally smooth, elliptical shape with a noticeable elongation. The central region exhibits a bright, concentrated core, suggesting a high stellar density or possibly an active galactic nucleus, though the resolution limits further conclusions. There's a radial color gradient, shifting from a yellowish-white core to a bluer hue toward the outer edges. This implies a potential distribution of younger, bluer stars in the surrounding regions compared to the older stellar population concentrated towards the center. No distinct spiral arms or prominent dust lanes are visible. There are no significant signs of tidal disturbances or ongoing mergers.
