The galaxy appears to be a spiral, exhibiting a prominent disk structure with well-defined spiral arms. These arms display a bluer hue, suggestive of ongoing star formation. A brighter, more concentrated central bulge is evident, with a color gradient towards a more yellow/red appearance. This suggests an older stellar population within the bulge. There appears to be evidence of interaction or disturbance. There are faint signs of tidal features, potentially indicative of a recent or ongoing merger event. The overall structure implies that this is a relatively massive, actively star-forming galaxy undergoing dynamic processes.
