The observed galaxy presents as a spiral galaxy with a prominent disk structure. The spiral arms appear well-defined and moderately wound, extending outwards from a central bulge. The bulge is of moderate size, not dominating the overall structure, and shows a smooth, yellowish hue, suggestive of an older stellar population. The spiral arms exhibit a bluer coloration, indicating regions of active star formation. There is evidence of at least two distinct spiral arms emanating from the central region. There's a hint of a bar-like structure in the central region, though not pronounced. The galaxy appears relatively undisturbed, without significant signs of major mergers or tidal disruptions. The disk is viewed at a slight inclination, revealing some of its three-dimensional structure.
