This galaxy appears to be a relatively smooth, elliptical or lenticular system. It exhibits a somewhat round morphology. The central region displays a bright, concentrated core that is mostly a red-yellow hue. The outer regions have a notable change to greener hues, suggestive of ongoing star formation. There is no distinct spiral structure visible, nor is there obvious evidence of significant tidal disturbances or ongoing major merger activity. The galaxy may have experienced minor merger activity based on some subtle irregularities in the outer regions. Overall, the galaxy presents a fairly regular and relaxed appearance, possibly indicating a relatively quiescent evolutionary state.
