The galaxy appears as a concentrated structure, potentially an early-type system. The light profile seems relatively smooth with no prominent spiral arms observed. The galaxy exhibits a moderate degree of central concentration, with the core region appearing brighter compared to the outer regions. The overall shape deviates from a perfect sphere, presenting an intermediate elongation. There is evidence suggesting possible interactions or minor disturbances present in the system, potentially indicating ongoing or past mergers. The galaxy's color suggests a stellar population dominated by older stars, consistent with low levels of current star formation. The overall morphology may be indicative of a galaxy in the process of assembly through mergers, or a system that has largely completed its formation and is now evolving passively.
