The galaxy presents a morphology indicative of a spiral type, though the spiral arms appear somewhat flocculent and not sharply defined. The arms emanate from a moderately sized central bulge that exhibits a yellowish hue, suggesting an older stellar population. The overall color of the galaxy is slightly bluer than the central bulge, hinting at ongoing star formation within the arms. No obvious bar structure is discernible. The galaxy appears relatively isolated, with no apparent signs of major mergers or significant tidal disturbances. A slight asymmetry is observed in the distribution of light within the arms, possibly indicating a minor interaction or internal dynamical processes. The galaxy's disk is viewed at a considerable angle away from edge-on.
