The galaxy presents as a singular, well-defined object. Its morphology appears largely smooth and elliptical, with no obvious spiral arms or distinct disk structure. The light distribution suggests a centrally concentrated spheroid shape, with a gradual decrease in luminosity outward from the core. The galaxy displays a color profile that leans towards the redder end of the spectrum, indicating a population of older stars and a relatively low rate of ongoing star formation. There is a subtle color gradient, with the central regions appearing somewhat yellower than the outer regions. No significant signs of tidal disturbances, merging activity, or prominent dust lanes are apparent. The galaxy seems to be undisturbed and exhibits a relaxed structure.
