The galaxy presents as a somewhat elongated structure with a significant central bulge. The morphology appears predominantly smooth, suggesting a relatively evolved system. The color profile indicates a redder central region, possibly indicative of an older stellar population. The outer regions exhibit a bluer hue, potentially signaling ongoing or recent star formation activity, with possible faint extended features. There is an indication of minor disturbances in the galaxy's form, possibly due to past interaction or internal processes. The overall structure does not appear to be undergoing a major merger.
