The galaxy presents an overall elliptical morphology, elongated along its major axis. It exhibits a generally smooth appearance, suggestive of an evolved stellar population. The central region displays a more concentrated and yellowish hue, potentially indicating a higher density of older stars and perhaps a supermassive black hole at the galactic nucleus. The outer regions show a bluer color, indicative of more recent star formation, although this feature is not strongly pronounced. There's some indication of a possible, though subtle, disk-like structure viewed at an angle. The galaxy does not appear to be undergoing any major merging events, though there might be a minor disturbance or faint tidal feature present. Star formation is still occurring at a relatively low rate.
