The galaxy presents a largely smooth, elliptical morphology with a slight elongation. The central region exhibits a bright, concentrated luminosity, suggesting a significant stellar density or a possible active galactic nucleus. The overall color appears to be yellowish-white, which could be indicative of an older stellar population, with a reduced rate of star formation. Faint, extended regions surround the central bulge, fading into the background, hinting at a gradual decrease in stellar density outward. A slight bluing of the light in the outer edges can be observed, implying some recent star formation or a population of younger, bluer stars in those regions. There appears to be a subtle hint of a disk structure, but it is not clearly defined. There is no obvious indication of spiral arms or significant dust lanes. No signs of ongoing major mergers are immediately apparent, but minor disturbances cannot be ruled out based on the image alone.
