The galaxy presents as a single, luminous object with a smooth, elliptical morphology. The color profile suggests an older stellar population. The primary color is a yellow-orange hue, intensifying towards the central region, indicating a potential concentration of evolved stars. The structure is centrally concentrated, with a gradual decrease in luminosity from the core to the outer regions. Faint hints of slightly less smooth patches or disturbances are suggested in the outer regions, perhaps indicating early stages of a minor interaction or past mergers. There appears to be a high degree of symmetry, with no obvious features such as spiral arms or a prominent disk. The overall impression is that of a quiescent galaxy, with minimal ongoing star formation.
