The galaxy presents as a spiral type, viewed at an oblique angle. It exhibits a prominent central bulge, though not dominating, which appears yellowish. Two distinct spiral arms are clearly visible, demonstrating a winding pattern from the core outward. A bar structure, if present, is weak. The arms display a mottled texture, suggesting regions of star formation. The outer regions of the disk appear fainter and bluer in color, indicative of a younger stellar population. No signs of major merging or tidal disturbances are evident. The overall shape approximates an ellipse, with a discernible flattening along its minor axis.
