The galaxy presents a relatively smooth, elliptical morphology. It displays a yellowish-orange color gradient, with the central region appearing brighter and more intensely colored, likely indicating a higher concentration of older stellar populations. The galaxy shows a slight elongation, deviating from a perfectly circular shape. There is a suggestion of subtle disturbances in its structure, possibly due to minor tidal interactions or internal processes. At least one diffuse object is present, in the vicinity of the galaxy, potentially indicating an ongoing merger or interaction with a smaller companion galaxy. There is a clear gradient in luminosity from the core to the outer edges, with a gradual fading into the background. The lack of distinct spiral arms or significant dust lanes suggests it is an evolved system, possibly with a low star formation rate.