The galaxy presents as a spiral type, exhibiting a discernible disk structure. The arms are prominent, with a relatively tight winding pattern. Two main spiral arms are clearly visible, emanating from the central bulge. A stellar bar appears to be present, though moderately defined, bisecting the bulge region. The central bulge is of a moderate size and exhibits a yellowish color, possibly indicating an older stellar population within it. The disk appears to be at a close to face-on orientation, as it displays a relatively circular shape. There is no obvious morphological distortion or signs of major interaction or merger events, though minor disturbances or tidal features are difficult to rule out at this resolution.
