The galaxy presents as a moderately bright object with a slightly elongated morphology. It appears to exhibit a disk-like structure, but significant disruption is evident, potentially resulting from tidal interactions or recent merger activity. The galaxy displays a relatively smooth central region with fainter, diffuse features extending outwards. The central region exhibits a slightly reddish hue while bluer regions are visible which suggests ongoing star formation. The overall light distribution suggests the galaxy is not perfectly symmetrical, further supporting the possibility of interactions or past mergers.
