The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high degree of luminosity, with a gradual decrease in brightness towards the outer edges. The light distribution suggests a predominantly older stellar population, with a yellowish hue dominating the visible spectrum. There is little evidence of spiral arms or significant dust lanes. The overall shape is nearly spherical, with a slight deviation suggesting a possible ellipsoidal form. Subtle irregularities in the outer halo may indicate past minor interactions, although no major merging events are readily apparent in the image. Star formation appears to be relatively quiescent within this galaxy.
