The galaxy presents a flattened, elongated morphology, suggestive of a disk-like structure viewed at an oblique angle. It appears relatively smooth in overall texture, though subtle variations in luminosity are discernable. The central region exhibits a brighter concentration of light, indicative of a possible bulge or nuclear component. The color profile suggests the presence of both older stellar populations, contributing to a redder hue in the central region, and a blue component, implying recent star formation activity, concentrated toward the outer disk. There is slight evidence of minor asymmetry or disturbance in the outer regions, possibly indicating interactions or past merger events. The overall structure can be characterized as a possibly disturbed disk galaxy.
