The galaxy presents as a moderately luminous object exhibiting a complex morphology. There is evidence of both a relatively smooth central component and distinct, seemingly disrupted features.

The central region appears diffuse and elongated, with a color gradient suggesting a mix of stellar populations. Fainter, bluer emissions are visible on the left-hand side of the core, indicating more recent star formation within the last few million years. Redder emissions appear in the lower central region of the galaxy, possibly indicating an older stellar population.

Extending outwards, the galaxy displays irregularities and distortions. Some of these features may be the result of tidal interactions or ongoing mergers. These could represent disrupted spiral arms, tidal tails, or debris from a smaller galaxy being accreted. The generally disturbed appearance of the galaxy suggests a dynamic environment and indicates recent or ongoing interaction with another galaxy.
