The galaxy appears as a centrally concentrated object with a smooth light distribution, indicative of an elliptical or lenticular morphology. There is a noticeable color gradient; the core region is a warm yellow-orange hue, which likely corresponds to an older stellar population and/or dust obscuration. Surrounding the core, there is a gradual transition to a greenish-yellow halo, which indicates the presence of younger stars. The galaxy's smooth profile and lack of prominent spiral arms suggest a relatively quiescent state. The galaxy does not appear to be undergoing a major merging event or experiencing significant tidal disturbances.
