This galaxy presents as a somewhat elliptical object with a notable central bulge. The light distribution is primarily smooth, indicating an older stellar population. There is some evidence of disk-like morphology, though it is not a dominant feature. The galaxy exhibits an orange-red hue, which is indicative of a population dominated by older stars. The galaxy does not present a classical spiral structure, but some disturbances could be signs of a minor merger. It is not perfectly round; it has a more oval shape. The galaxy shows a relatively compact core.
