The galaxy presents as an elliptical morphology, devoid of prominent spiral arm structures. The light distribution appears relatively smooth and centrally concentrated, exhibiting a gradual decrease in surface brightness from the core to the outer regions. The galaxy exhibits a moderate apparent size, and its color profile indicates a generally older stellar population, with a subtle shift toward redder wavelengths. There is little evidence of recent major merger events. Possible minor disturbances could be suggested by subtle asymmetries in the outer halo region. Overall, the galaxy appears to be a relatively quiescent system.
