The galaxy presents a morphology that is largely smooth and elliptical, exhibiting a concentrated central bulge region with a noticeable yellow-orange hue. This suggests an older stellar population, where star formation is subdued. A fainter and more diffuse reddish extension is visible on one side, possibly representing a tidal tail or a minor disruption, however it is more likely just a difference in stellar population. The galaxy appears to be mostly undisturbed with no major mergers or activity observed. The shape is somewhere between round and elongated, but not a significant cigar shape.