The galaxy presents as a singular, relatively smooth object. Its overall shape is elliptical, with a suggestion of elongation along one axis. The central region exhibits a brighter, more concentrated intensity of light, suggesting a higher density of stars or a possible active galactic nucleus, though further spectral analysis would be required to confirm. The color appears to be a faint blue hue overall. There are no apparent spiral arms or distinct dust lanes visible within the galaxy. The outer edges of the galaxy gradually fade into the background, indicating a diffuse stellar halo. There is a subtle irregularity in the shape, possibly indicating a minor gravitational interaction or disturbance in the recent past. The absence of clear merging features suggests that this is not a major ongoing merger event.
