The galaxy presents a generally smooth, rounded morphology. The light distribution is concentrated towards the center, with a bright, relatively compact core. There is evidence of color variation, with a bluer hue prominent in the central region, transitioning to redder tones in the outer regions. This color gradient suggests a differential stellar population, with potentially younger, hotter stars concentrated in the center and older, cooler stars distributed in the periphery. There appears to be a slight asymmetry and some subtle disturbances of what would otherwise be a smooth light profile.