The galaxy appears as a relatively faint and diffuse object. Its overall color seems reddish, with a hint of bluer regions within. The light is not uniformly distributed, suggesting some degree of substructure. However, there is no clear indication of a well-defined spiral arm structure, bar, or prominent central bulge. The overall morphology is somewhat irregular. There seems to be a slight disturbance in the outer edges with a faint plume or tail-like feature extending away from the main body, potentially indicative of a past or ongoing interaction or merger. The galaxy seems to be mostly isolated, and the feature could also be caused by gas stripped away due to the galaxy's movement through the intergalactic medium.
