This galaxy exhibits a disturbed morphology, likely indicative of a merger event. The light distribution reveals two distinct, yet overlapping, luminous regions. The primary nucleus appears yellowish-orange, suggesting a population of older stars. A secondary concentration of light, also yellowish, is observed in close proximity, further supporting the interpretation of an ongoing or recent merger. Diffuse blue light is present, intermixed within the galaxy, indicating regions of active star formation. The overall shape is irregular, lacking a well-defined spiral or elliptical structure. The tidal features, while faint, extend from the main body, suggestive of gravitational interaction and disruption.
