This galaxy presents as a relatively smooth, luminous structure. It exhibits an elliptical morphology, with a high degree of central concentration. The light distribution suggests a predominantly older stellar population. The color profile is somewhat homogenous across the galaxy's body, except for a slight bluing in the outer regions. There is an indication of ongoing star formation in the outer regions, possibly leading to minor disturbances in the otherwise smooth morphology. Overall, this galaxy appears to be a quiescent system with evidence of past merger events.