The galaxy presents as a diffuse, relatively faint object, with a reddish hue becoming apparent in the faint light from the galaxy. While a distinct structure is difficult to discern, the light distribution suggests the possible presence of a distorted disc, with faint wisps or tails extending outwards. There appears to be a possible tidal feature in the northern part of the galaxy. The light is concentrated in the central area with the intensity quickly decreasing with the increasing radius, suggesting possible old stellar population. There is no easily distinguishable spiral structure or bar. The overall morphology implies that the galaxy could be undergoing or has recently undergone a merger. Further investigation with deeper imaging and spectroscopic data would be beneficial to confirm these initial observations and determine the precise nature of the observed distortions.
