The galaxy presents a largely smooth, elliptical morphology, with a noticeable lack of distinct spiral arms or a prominent disk structure. The central region exhibits a diffuse glow, suggesting a high concentration of stars. There appears to be a slight elongation along one axis, deviating somewhat from a perfectly circular shape. There is an area to the side of the galaxy that indicates some disturbance and may represent a minor merging event. The colors are generally muted, with a subtle shift toward redder hues. Overall, the galaxy's characteristics point towards an older stellar population and relatively low levels of ongoing star formation.
