The galaxy presents as a slightly elongated structure with a predominantly smooth morphology. Its color profile appears to shift from a yellowish hue at one end to a bluer tint at the opposite. This color gradient possibly indicates differing stellar populations or varying dust content across the galaxy's extent. There is a subtle suggestion of a disk-like component but it isn't clear. Evidences of any significant recent merging events are not apparent, despite the somewhat irregular shape, suggesting a relatively settled state. However, a minor gravitational interaction might not be ruled out without more detailed analysis. The galaxy appears relatively compact, with no obvious extended halo or tidal features visible in the immediate vicinity.
