The galaxy presents as an elliptical-like structure, appearing moderately smooth and with a disk component. The central region exhibits a concentrated luminosity, suggesting a substantial bulge. The overall shape is somewhat elongated, with an axis ratio indicating a deviation from a perfect sphere. There is subtle evidence of possible minor disturbances in the outer regions, and a lack of a clear spiral arm structure. Color gradients suggest a population gradient, with a redder central bulge and slightly bluer outer regions. The galaxy is estimated to be fairly massive with moderate star formation activity.
