The galaxy presents as a spiral galaxy with a redshift of approximately 0.024, indicating a relatively nearby object. It exhibits a prominent central bulge that appears moderately bright and concentrated. The disk component shows a developed spiral structure, characterized by tightly wound arms. These arms are prominent and contribute significantly to the overall light distribution of the galaxy. There is no strong evidence of a bar structure bisecting the central bulge.

The galaxy appears relatively undisturbed, showing no signs of major merging or tidal distortions. The spiral arms lack significant irregularity or truncation, indicating the absence of recent major interactions with other galaxies. The size of the galaxy is typical for a spiral, with the disk extending a considerable distance from the central bulge.
