The galaxy presents as an elliptical morphology, appearing largely smooth and featureless in this image. It exhibits a concentrated central bulge, with a gradual decrease in luminosity towards its outer regions. There is a yellow-reddish hue, suggestive of an older stellar population, and potentially lower rates of current star formation. The galaxy's overall shape is roughly elliptical, although there are hints of asymmetry, perhaps due to minor gravitational interactions or internal dynamics. There is a suggestion of a fainter and smaller companion galaxy nearby. No prominent dust lanes or spiral arm structures are evident within the limitations of this image resolution. The galaxy seems to be neither an actively merging system nor undergoing major structural disruption.
