The galaxy presents as a barred spiral with a moderately sized bulge. The bar appears prominent, exhibiting a bright, yellowish hue that blends somewhat seamlessly into the central bulge. Spiral arms emanate from the ends of the bar, loosely winding outwards. A primary structure containing two dominant spiral arms is observed. These arms exhibit a mottled appearance, suggestive of varying stellar densities and potential star formation regions. The overall color profile indicates a relatively mature stellar population, with a leaning towards redder wavelengths dominating the light emitted from the central regions. Distortions in the shape of the arms, particularly near the outer edges, may suggest some gravitational interaction. Although no significant disturbances are clearly visible.