The galaxy presents as a slightly elongated, diffuse object with a predominantly bluish central region. Its overall structure appears relatively smooth with some subtle irregularities in the light distribution. The galaxy shows a slight disk-like structure, however this is disturbed. There is no dominant central bulge. The outer edges gradually fade into the background, indicating a lack of a sharp boundary. There may be some evidence of past mergers and/or some interactions due to the disrupted disk structure.
