The galaxy presents a generally smooth, elliptical morphology. Its shape is slightly elongated, showing an intermediate degree of roundness, and it does not appear to be highly flattened or cigar-shaped. The central region exhibits a concentrated brightness, suggesting a substantial stellar population. The galaxy displays a noticeable color gradient, with a yellowish core transitioning to redder hues toward the outer regions. There is no prominent evidence of spiral arms or significant dust lanes. There are no clear signs of major mergers or strong tidal disturbances affecting the galaxy's overall structure, although a potential minor disturbance is not fully ruled out. The galaxy's estimated size indicates it is a substantial object, even at a significant distance.
