The galaxy presents a relatively bright central bulge that appears moderately sized in comparison to the overall galactic structure. Faint spiral arms emanate from the central region, appearing somewhat diffuse and open in their winding. The arms exhibit a mottled texture, suggesting the presence of active star formation regions or dust lanes. There is a distinct lack of a strong central bar feature. The overall color profile reveals a subtle gradient, transitioning from a yellowish hue in the bulge to a bluer tint in the outer spiral arms, indicative of a mixed stellar population and ongoing star formation. There is a noticeable degree of disturbance, suggesting possible interactions, but not to the degree where a merger is readily apparent. 
