The galaxy presents a somewhat elliptical morphology. The light distribution appears relatively smooth and concentrated towards the center, suggesting a prominent bulge. There is some evidence of a faint, diffuse disk surrounding the bulge. The color gradient shows a redder hue in the central regions, indicative of an older stellar population, while the outer regions exhibit a bluer tint, potentially suggesting younger stars or ongoing star formation, albeit at a low rate. No strong spiral arms or major disturbances are readily apparent. The overall structure appears relatively undisturbed, without any obvious signs of a major ongoing merger. The galaxy's profile suggests a transition type between a pure elliptical and a fully developed spiral.
