This galaxy presents a roughly elliptical morphology, exhibiting a noticeable disk structure. The central region displays a bright, concentrated core, suggestive of a significant stellar population and possibly an active galactic nucleus. The disk appears relatively smooth with some subtle deviations in color and brightness. The colors suggest regions of active star formation, particularly within the disk, possibly indicative of spiral arm structures that are not immediately apparent. There is a slight distortion of the overall shape, suggesting a minor gravitational interaction or past merger event influencing its current morphology. The object shows faint extended features indicating the presence of a galactic halo. Overall, the galaxy appears to be an intermediate-mass system.
