The galaxy presents as a largely featureless, elliptical form, exhibiting a high degree of radial symmetry. The light profile is dominated by a bright, centrally concentrated core that diffuses outward into a more indistinct halo. The color gradient suggests a population of older stars throughout, with the central region appearing slightly more yellow, possibly indicating a higher concentration of evolved stars. There is a very slight suggestion of a disk, although it is difficult to be certain. There is no evidence of significant dust lanes, spiral arms, or ongoing major merger activity. Overall, the galaxy appears to be an early-type system with a relatively smooth and relaxed morphology.
