This galaxy exhibits a generally elliptical morphology, though it is not perfectly round. A diffuse, extended halo surrounds a brighter central region. Within the halo, there is some indication of faint, broad spiral arm-like structures, suggesting a possible disk component. The color gradient transitions from a slightly bluer hue in the outer regions to a yellower color towards the center, indicating a potential change in stellar populations. There is a localized area of intense blue/green light in the disk region on the side of the galaxy, indicating possible star formation. Based on the disturbance fraction, there is evidence of minor interactions but there are no clear signs of major mergers or tidal tails visible in the image.
