The galaxy presents as a moderately bright, somewhat diffuse object, with an elliptical morphology. It appears largely smooth in texture, with a high degree of roundness. There is a subtle color gradient, with a slightly more yellowish hue towards the central region, suggesting an older stellar population concentrated in the core. The outer regions exhibit a bluer tone, potentially indicating the presence of younger stars, or ongoing, if limited, star formation. There is a slight asymmetry to the light distribution, possibly indicative of a minor interaction or past merger event, although no clear tidal tails or other signs of major disturbance are readily apparent. The galaxy does not display prominent spiral arms or a distinct disk-like structure.
