The galaxy presents an overall elliptical morphology, with a concentrated, bright nucleus. The light distribution appears relatively smooth, with a gradual decrease in intensity from the core outwards. There is a subtle elongation in the galaxy's shape, suggesting it is not perfectly spherical. There are faint hints of a possible disk-like structure or spiral arm fragments within the outer regions, though these are not sharply defined. The galaxy exhibits a color gradient, with the central region appearing yellower, likely indicating an older stellar population, while the outer regions appear slightly bluer, hinting at the presence of younger, hotter stars and the potential for ongoing, albeit low, star formation. There is no obvious indication of strong tidal interactions or major mergers occurring within the galaxy.
