The galaxy presents a somewhat diffuse, irregular morphology. The overall structure appears disturbed, possibly indicative of gravitational interactions or a recent merger event. There are no clearly defined spiral arms or a prominent central bulge. The light distribution is uneven. Some regions show slightly brighter and more concentrated emission, while others appear fainter and more spread out. The galaxy exhibits a reddish color. This suggests a population of older stars and/or significant dust obscuration, possibly inhibiting the light of any young stars that may be present. There is some evidence of minor tidal tails or asymmetries in the outer regions, further supporting the hypothesis of past or ongoing gravitational interactions.
