The galaxy presents a well-defined disk structure viewed at an intermediate inclination angle. There is evidence of spiral arm morphology but the features appear somewhat flocculent and not highly organized. A prominent central bulge dominates the luminosity profile, with the light appearing more concentrated than the surrounding disk. The bulge has a smooth texture with a yellowish hue indicating an older stellar population. A bar-like structure appears to traverse the central region of the galaxy, bisecting the bulge along its major axis. The disk component exhibits a bluer color, suggesting ongoing star formation. There do not appear to be any major disturbances or signs of recent mergers. The overall structure points toward it being a barred spiral galaxy.
