The galaxy presents as a moderately concentrated, somewhat smooth structure. The overall morphology appears roughly elliptical. A diffuse halo of light surrounds the central region, exhibiting a gradual decrease in surface brightness with increasing radial distance. There is a possible faint tidal tail feature. The color profile suggests a predominantly older stellar population, as indicated by the reddish-yellow hues dominating the central bulge and the extended halo. Evidence suggests that this galaxy is undergoing a significant merger event. There is a notable disturbance in the overall morphology with a large amount of luminous matter located within the central structure.
