The galaxy exhibits a moderately bright core region. Morphologically, the object appears relatively smooth, with a slight central bulge and a surrounding disk. There are hints of minor disturbances in the morphology. The galaxy appears to be undergoing a minor merger with a potential galaxy nearby. There may be an object close to the galaxy exhibiting interactions. The main body of the galaxy demonstrates a color gradient, with bluer hues concentrated towards the center. This may indicate active star formation within the central region. The outer regions of the galaxy appear redder, possibly indicating an older stellar population. Overall, the galaxy presents as a dynamically active system with evidence of interactions and ongoing star formation.
