The galaxy presents as a disturbed system, potentially undergoing a merger. A central, somewhat amorphous bulge is visible, displaying a yellowish hue, suggesting a population of older stars. There are two other distinct objects, one above and one below, that are much smaller and less illuminated. These are interacting with the main galaxy body. The morphology is neither clearly spiral nor elliptical, showing irregular features indicative of ongoing gravitational interactions. There is a faint halo-like component surrounding the galaxy. The overall light distribution is not uniform, showing complex and perturbed features, suggestive of tidal effects. Evidence indicates a low star formation rate.
