The galaxy presents as a spiral type, exhibiting a distinct disk structure. The disk is viewed at an oblique angle, not quite edge-on but significantly tilted from a face-on orientation. Spiral arms are discernible, appearing tightly wound around a central bulge. The bulge itself presents with a moderate size. A hint of a bar feature appears weakly in the central region. Star formation appears to be present, but perhaps not dramatically active, and is observed throughout the spiral arms. The color profile suggests a mature stellar population, though some blue regions indicate ongoing star formation. There may be some evidence of a minor interaction or disturbance in the disk, though the galaxy's overall morphology remains largely undisturbed.
