The galaxy presents as a spiral, observed at an oblique angle relative to our line of sight. Two prominent spiral arms are clearly visible, winding moderately tightly around a bright central bulge. This central bulge appears significant in size, exhibiting a moderate contribution to the overall galactic luminosity. A bar structure is faintly suggested within the central region, though it isn't overwhelmingly defined. The overall disk of the galaxy appears relatively smooth with only slight disturbances in the morphology. The color distribution suggests a mix of stellar populations, the central bulge appearing yellower, potentially indicative of older stars, while the spiral arms have a bluer hue, possibly signaling ongoing star formation. Overall, the galaxy is not undergoing any significant merging activity and has no major morphological disturbances.
