The galaxy presents a somewhat smooth, elongated morphology. The light distribution is concentrated towards the center, suggesting a prominent bulge. It exhibits a general blueish hue, with some variations in intensity, especially around the core region, which can be due to a population of relatively young, hot stars. The outer regions are fainter and bluer compared to the central bulge, which shows a whiter tint. Overall, the galaxy appears relatively undisturbed, with no apparent signs of major mergers or strong tidal interactions.
