The galaxy presents a roughly elliptical morphology, with a high degree of central concentration. The core exhibits an intense, bright emission, potentially indicating a highly active galactic nucleus or a region of intense star formation. The radial color profile suggests variations, transitioning from a predominantly blue-green hue in the central region to a slightly redder tint towards the outer edges, possibly indicative of an aging stellar population in the outskirts. There appears to be a level of morphological disturbance, which may be caused by a merging event. The galaxy appears to be a singular entity; there are no indications of companions or multiple nuclei. 
