The galaxy presents a complex morphology, suggestive of a recent or ongoing interaction or merger. The central region is dominated by a bright, concentrated bulge, exhibiting a yellowish hue. This may indicate an older stellar population within the bulge. Extending outwards from the central bulge, there are notable structures that appear to be disrupted spiral arms. These arms are traced by regions of bluish light, potentially indicative of active star formation within them. The overall structure of the galaxy is distorted, lacking the clear symmetry often observed in undisturbed spiral galaxies. There are significant asymmetries and irregularities in the distribution of light, particularly within the outer regions of the disk. A faint tidal tail can also be seen, suggesting gravitational interaction with a smaller galaxy nearby.
