The galaxy presents a disturbed morphology, suggestive of an ongoing or recent merger event. The light distribution is irregular, with no clear central bulge or spiral arm structure discernible. The central region appears to be dominated by a bright, concentrated source with a yellow-orange hue, potentially indicative of an older stellar population and/or dust obscuration. Extending outward from this central region, diffuse blue patches are observed, which could signify regions of active star formation where hot, young stars are abundant. Fainter reddish regions are also present, potentially containing dust. The overall shape is asymmetric and elongated, deviating significantly from a typical elliptical or spiral galaxy. The apparent lack of a well-defined structure, coupled with the presence of star-forming regions and the suggestion of a merger, implies a dynamically active system, far from equilibrium. Further analysis is needed to confirm the nature and age of the stellar populations, the mass distribution, and the kinematic properties of the galaxy.
