The object presents as a spiral galaxy, oriented at a moderate inclination relative to our line of sight.  The central bulge appears prominent and exhibits a smooth, yellowish color gradient, indicating an older stellar population likely dominated by red giant stars.  Spiral arms are visible, originating close to the bulge and extending outwards.  The arms display a patchy distribution of bluer regions suggestive of ongoing star formation within HII regions. The spiral arms appear bifurcated, and have intermediate winding. There appears to be a minor interaction or disturbance in the structure, possibly a tidal tail or asymmetry in the outer disk. The galaxy displays an overall ordered structure, with no signs of a major merger event disrupting its morphology.
