The galaxy presents a relatively smooth morphology, appearing largely elliptical in shape, elongated at approximately a 20-degree angle relative to the image's horizontal axis. The core is significantly brighter and more condensed than the outer regions of the galaxy. The galaxy exhibits a radial color gradient, with the central region appearing bluer and the outer edges becoming progressively redder, indicating a possible difference in stellar populations. The lack of distinct spiral arms or prominent dust lanes suggests it is not a spiral galaxy, and instead a likely early-type galaxy. There is a slight irregularity in the outer halo, hinting at a possible minor disturbance or past interaction.
