The galaxy presents as a moderately bright, elliptical formation. Its core is highly concentrated with light, appearing nearly spherical, while the outer regions show a decrease in luminosity, with the overall shape being somewhat elongated. There is a relatively smooth light distribution throughout the galaxy, suggesting a lack of significant spiral arms or patchy dust lanes. The galaxy's color suggests a population of older stars; there is a slightly bluer tint in the center, although this could be due to issues with the image. Overall, the galaxy seems to be relatively isolated, with no obvious signs of tidal interactions or major disturbances in its morphology. The absence of visible substructure indicates a fairly evolved and relaxed stellar system.
