The galaxy appears to be a merging system. A primary, more massive galaxy is visually dominant with a relatively smooth, centrally concentrated light distribution. This main galaxy shows a slight elongation but is generally rounded in shape. There is a secondary object in proximity to the primary galaxy, showing a fainter, more diffuse structure. There's an indication of tidal disturbance or interaction between the two, potentially a tidal tail or bridge of material connecting or distorting their shapes. The colors suggest a range of stellar populations; the primary galaxy shows a higher concentration of redder hues at its core, possibly indicating an older stellar population. The outer regions appear slightly bluer, suggesting more recent star formation. The galaxy has an estimated size of a few kiloparsecs.
