The galaxy appears to be a relatively smooth, elongated system, seen at an oblique angle. Its overall shape is reminiscent of a flattened spheroid, possibly a disk galaxy viewed nearly edge-on. The central region exhibits a higher surface brightness, suggesting a concentration of stars towards the galactic nucleus. There is a subtle color gradient across the galaxy, with the central regions possibly appearing more yellow or orange, transitioning to a slightly bluer hue towards the outer regions. The galaxy exhibits some minor disturbance, but not in a strong or chaotic manner. There is no indication of major merging activity, such as strong tidal tails or distorted morphology.
