This galaxy appears to be a relatively smooth, disk-shaped structure, with an elliptical morphology. The central region exhibits a concentrated, bright core, possibly indicative of an older stellar population. The overall color profile suggests the presence of both younger, bluer stars, particularly in the outer regions, and older, redder stars concentrated towards the center. There is some indication of a faint, disk-like structure extending beyond the central bulge, however there are no clear spiral arm structures or distinct features suggesting a strong ongoing star formation. The galaxy shows a slightly elongated shape, which could be due to an inherent asymmetry or a viewing angle that is not perfectly face-on. There are no obvious signs of major mergers or significant tidal disturbances.
