The galaxy presents as a spiral type, displaying a clear disk structure. This disk is not perfectly face-on, exhibiting a slight tilt relative to the observer's line of sight. Two prominent spiral arms emanate from a central bulge, winding moderately outwards. The arms appear somewhat fragmented, indicating regions of active star formation. The central bulge seems small relative to the overall disk size. A faint bar-like structure can be inferred across the bulge region. There are no obvious signs of ongoing major mergers. However, there is some subtle irregular structure that might indicate minor tidal disturbance. The color distribution suggests a mixture of stellar populations, with a concentration of yellow light in the core indicative of older stars, and bluer colors in the spiral arms associated with younger, massive stars.
