The galaxy presents as a single, relatively smooth object, exhibiting a pronounced elliptical morphology. The luminosity profile appears centrally concentrated with a gradual decrease in brightness outwards. The primary color is a yellowish hue, indicating a significant population of older stars. There is no obvious indication of spiral arms or a prominent disk structure. Faint blueish patches are visible towards the core, possibly indicating a slight presence of younger stars. No signs of significant tidal disturbances or ongoing major mergers are readily apparent, although a slight asymmetry is visible. The overall appearance suggests an evolved system with relatively low levels of current star formation activity.
