The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a predominantly elliptical morphology, with an intermediate apparent roundness. There is no clear evidence of spiral arm structure or a prominent disk component. The galaxy's light profile appears to lack significant distortions or tidal features suggesting it is not undergoing a major merging event, but there might be minor disturbances in the surrounding stellar structure. The galaxy appears to have a low star-formation rate. The core exhibits a slightly redder hue, possibly indicative of an older stellar population. The overall color index suggests a relatively evolved system.
