The galaxy presents as a generally smooth, elliptical-like structure. The light profile appears concentrated towards the center with a gradual decrease in intensity outwards. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. No distinct spiral arms or dust lanes are readily visible, and the overall morphology indicates a lack of major ongoing star formation. There may be slight disturbances or minor asymmetrical features in the outer regions of the galaxy, but these are faint. The galaxy has a slightly elongated shape.
