The galaxy presents a generally smooth and somewhat elongated morphology. The central region exhibits a higher surface brightness, appearing as a concentrated bulge. The color profile suggests the presence of both older stellar populations, indicated by a slightly redder hue in the outer regions, and relatively younger, hotter stars that give off a bluer color. The disk itself is not clearly resolved. The overall structure indicates a system that is not undergoing significant, current major merging events. There is little indication of strong tidal features, though subtle asymmetric distortions cannot be ruled out given the image resolution. Based on its apparent color gradient, it would appear to be a system with moderate ongoing star formation.
