The galaxy presents an elliptical morphology, appearing largely smooth and featureless. There is a concentrated central bulge exhibiting a yellowish-white hue, indicative of an older stellar population. The overall shape is somewhat elongated but not highly cigar-shaped; it could be described as being somewhere between round and elongated. There's a subtle color gradient extending outwards from the core, with the outer regions showing a slight bluer tint, possibly indicating pockets of younger stars or ongoing star formation at a low rate. No strong evidence of spiral arms or a disk structure is visible. There are no obvious signs of a major ongoing merger, however, there is a slight perturbation on one edge, indicating the possibility of a minor disturbance, perhaps from a past or distant interaction. The light is relatively even throughout, indicating that the galaxy is well settled.
