The galaxy appears to be an elliptical or lenticular type. It presents a generally smooth morphology with a central bulge that is brighter and more concentrated. There is no distinct spiral arm structure evident. The color profile suggests an older stellar population, with reddish hues dominating, especially within the central bulge. Fainter, bluer light is present in the outer regions, perhaps indicating some ongoing, albeit low, star formation in the galaxy's disk or outer halo. There appears to be some minor disruption in the outer parts of the galaxy. Overall, the galaxy exhibits a morphology consistent with a relatively evolved system.
