The galaxy presents a generally smooth, elliptical morphology. There is no visible spiral structure or distinct disk component. The central bulge is prominent and exhibits a bright, concentrated luminosity. The radial light profile suggests a gradual decrease in brightness from the core outwards. The galaxy appears to be relatively isolated, with no immediately obvious signs of major interactions or ongoing merging events, though there is a minor possibility of disturbance. Color gradients suggest a population of older stars.
