The galaxy presents a generally smooth, elliptical morphology. The light is concentrated in the center and fades gradually into the surrounding space. The galactic core appears bright with a yellow hue suggesting an older stellar population with minimal ongoing star formation. Fainter blue-ish light is visible around the nucleus, potentially indicative of a younger stellar population. The galaxy shows a high degree of roundness. No distinct spiral arms or bar structures are visible. The overall appearance suggests that this galaxy has not recently undergone any major merging events or significant gravitational disturbances.
