The galaxy exhibits a morphology suggestive of an ongoing or recent merger event. The central region displays a concentrated bright core, possibly indicative of an active galactic nucleus or a dense stellar population. Surrounding the core, there is evidence of disturbed morphology. Faint tidal features or extended arms are not clearly present, however the fuzzy appearance of the galaxy as a whole suggests interaction with a small companion.

The color of the central region is weighted toward the blue end of the spectrum. This bluer color suggests ongoing star formation. The overall luminosity of the galaxy appears significant.
