This galaxy appears to be undergoing a merger event. The system presents with an elongated morphology. The primary component is a concentrated, centrally brightened spheroid exhibiting a yellowish-white color profile, suggesting a population of older stars. Extending outwards from this central region are diffuse, bluish structures, possibly indicative of ongoing or recent star formation. A secondary object, smaller and more compact, is visible; it is redder in color, potentially due to a high dust content or an older stellar population, and appears connected via a faint bridge of material to the primary galaxy. This morphology suggests an interacting system, possibly in the late stages of merging. The overall structure is disturbed, lacks well-defined spiral arms, and shows irregular light distribution.
