The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears largely elliptical. There is a distinct color gradient, shifting from a bluer hue in the outer regions to a redder, more yellowish color towards the core. The central region is significantly brighter than the outer disk, suggesting a higher concentration of stars. There is no readily apparent spiral structure or bar feature visible. The galaxy displays no signs of significant tidal disturbance or ongoing merger activity in this image. Faint irregular features, such as tidal tails or shells, are absent. The overall morphology suggests a galaxy with a population of older stars.
