The galaxy presents as a spiral-type morphology, though somewhat face-on relative to our line of sight. The central bulge appears prominent and exhibits a yellowish-white color, indicative of an older stellar population. Spiral arms are visible, displaying a mottled appearance with blueish regions possibly suggesting ongoing star formation. The arms are not tightly wound, showing a somewhat flocculent structure. The galaxy's overall color is dominated by intermediate wavelengths, with redder hues concentrated in the bulge and bluer colors appearing in the arms. There is no obvious evidence of a major merger or significant tidal disruption, although some minor asymmetries in the spiral arms could suggest past interactions. The disk appears relatively smooth without major starburst regions visible. The object is elongated, but not overly so, and its isophotes gradually fade into the background sky, indicating no sharp truncation of the disk.
