This galaxy appears to be a relatively compact system, with a somewhat irregular morphology. There is evidence of a disk-like structure, although this is significantly disturbed, possibly indicative of a past or ongoing interaction. A component of this galaxy may have a smooth, possibly spheroidal morphology. The galaxy displays a broad color gradient, with bluer regions and what appears to be a redder center. The blue color suggests ongoing star formation, though at a modest rate. The redder hue implies an older stellar population. A faint tidal tail, or other form of disruption, cannot be entirely ruled out. There are potentially interactions and merging activity ongoing.
