The galaxy presents as a spiral type, exhibiting a central bulge of concentrated luminosity that gradually diminishes outwards. Faint spiral arms emerge from the central region, loosely winding around the core. The colour profile indicates a yellowish central bulge, potentially signifying an older stellar population, while the spiral arms display subtle hints of blue, suggesting more recent star formation. The galaxy appears relatively undisturbed, with a well-defined disk structure and no obvious signs of recent major mergers or tidal distortions.
