The galaxy presents a generally smooth morphology. The light distribution appears centrally concentrated with a moderate degree of ellipticity, showing a slight deviation from a perfectly circular shape. The galaxy exhibits a color gradient, with a central region appearing more red compared to the outer regions of the galaxy. There are faint hints of possible disturbances or asymmetries in the galactic structure, with a slight elongation suggesting a potential interaction or merging event. The overall color suggests an older stellar population and a relatively low star formation rate.
