The galaxy appears as a largely featureless, elliptical or spheroidal structure. It exhibits a smooth, centrally concentrated luminosity profile. The central region displays a yellowish hue, suggesting a population of older stars. The overall shape is predominantly round, with minimal discernible deviations from elliptical symmetry. There is no clear evidence of spiral arms or a pronounced disk component. A slight extension or asymmetry might be present in the outskirts, but the image resolution limits a definitive determination. The galaxy appears to be relatively isolated, with no obvious signs of major ongoing interactions or mergers with other galaxies.
