The galaxy appears as a somewhat elongated, diffuse object. The overall color gradient indicates a central concentration of older stellar populations, exhibiting a yellowish hue. A secondary, more reddish concentration is observed slightly offset from the main galactic nucleus. The morphological structure suggests a possible interaction or merger event, with the reddish concentration possibly representing a tidally disrupted dwarf galaxy or a region of intense star formation triggered by the interaction. There is limited evidence of distinct spiral arm structure or a well-defined disk, suggesting that if it is present it is being disrupted. The overall smoothness of the light distribution suggests that the system may be in a relatively advanced stage of merging, where distinct features are being blurred through tidal forces. The galaxy is of intermediate size.
