The galaxy presents as a single, largely featureless elliptical object. It exhibits a high degree of central concentration, with luminosity decreasing smoothly outward from the core. No distinct spiral arm structures or bar features are discernible. The galaxy's light profile appears roughly circular, showing little indication of ellipticity or asymmetry, suggesting it has not undergone any major merging events recently. Color gradients within the galaxy are subtle, but the central region appears somewhat yellower than the outer regions, suggesting an older stellar population in the core. Overall, the galaxy appears to be a relatively quiescent system, potentially with a low rate of ongoing star formation.
