The galaxy presents a generally smooth, elliptical morphology. The light is concentrated towards the center, with a gradual decrease in intensity outwards. The core exhibits a yellowish hue, potentially indicating an older stellar population. There are minimal apparent features such as spiral arms or dust lanes visible in this image, contributing to the overall smooth appearance. There is no apparent evidence of tidal disturbances or recent major mergers. The roundness and lack of significant asymmetry reinforces the smooth, elliptical classification.
