The galaxy presents a generally smooth and rounded morphology. There is little evidence of spiral arm structure or a prominent disk. The light distribution appears concentrated towards the center, fading gradually outward. A slight elongation is suggested, but the overall shape is predominantly round, with possibly some disturbances. There appear to be some nearby galaxies possibly merging with this primary galaxy. The galaxy has a redder hue, suggesting a population of older stars, but there also appears to be some blue areas in the galaxy which could mean ongoing star formation.
