The galaxy exhibits a generally smooth morphology, lacking prominent spiral arms or a strong bar structure. It appears largely elliptical in shape, with a high degree of central concentration. The core is bright and yellowish-white, suggesting an older stellar population and minimal ongoing star formation. The outer regions of the galaxy fade gradually, exhibiting a slightly bluer hue compared to the core, possibly indicative of a small population of younger, bluer stars. There is no visually apparent evidence of significant tidal disturbances, ongoing mergers, or pronounced disk-like features. The galaxy appears largely undisturbed, consistent with a relaxed system that has undergone significant evolutionary processes.
