The object presents as a spiral galaxy, likely at a redshift of approximately 0.06. It exhibits a distinct disk structure, observed nearly face-on. The spiral arms are prominent, well-defined, and tightly wound around a central bulge region. Two dominant spiral arms are clearly visible. The bulge appears relatively small compared to the overall disk size. Star formation appears concentrated within the spiral arms. There is evidence of a stellar bar that extends through the bulge region. The system displays some signs of gravitational interaction, though not overwhelmingly disturbed, indicative of either a minor interaction or an early stage of merging with another galaxy. The system is relatively compact, with a diameter on the order of a few kiloparsecs.
