The galaxy presents a disk-like structure, inclined relative to our line of sight. Spiral arms are evident, displaying a moderate winding pattern. Two dominant arms can be discerned. The central region appears to host a bulge of moderate size, possibly harboring an active galactic nucleus or a significant population of older stars, given its relatively smooth appearance. Star formation appears to be present within the spiral arms, as indicated by the blue hue. There is no strong evidence of a bar structure. The galaxy appears relatively undisturbed, with no significant signs of recent major merging activity. However, some minor irregularities in the disk structure could suggest a past minor interaction or accretion event. Overall, the galaxy appears to be a spiral galaxy in a relatively stable evolutionary state.
