The galaxy presents as a slightly inclined spiral type. Well-defined spiral arms are visible, extending from a moderately bright central bulge. There is evidence of a bar-like structure running through the central region. The arms appear somewhat flocculent, with a noticeable presence of star-forming regions indicated by their bluer color. The overall color of the galaxy indicates a mix of stellar populations, with the central bulge displaying a slightly redder hue, suggestive of older stars, and the spiral arms exhibiting a bluer cast, pointing towards younger, hotter stars. There is no strong evidence of major mergers or significant tidal disturbances.
