The galaxy appears to be undergoing a merger. There is evidence of two distinct nuclei within a common, disturbed halo of stellar material. The primary nucleus exhibits a yellowish-white color, suggesting a population of older stars and possibly dust obscuration. A secondary, smaller component is visible near the primary nucleus, displaying a bluer hue. This bluer color indicates the presence of a younger stellar population, possibly triggered by the merger event.

The overall shape of the galaxy is irregular, deviating significantly from a classic elliptical or spiral morphology. A faint tidal tail or bridge-like structure seems to extend away from the main body, further indicating gravitational interaction and disruption. The galaxy's luminosity is concentrated towards the central regions, but there's a general fuzziness around the edges. Overall, the galaxy's morphology is complex and indicates a system experiencing a significant gravitational interaction.
