The galaxy presents as a somewhat elongated structure, possibly indicative of a disk galaxy viewed at an oblique angle. The central bulge appears bright and yellowish, which could point to an older stellar population dominating the core. Moving outwards from the bulge, a fainter, bluer region is visible. This suggests ongoing star formation within the galaxy's disk. There is an indication of a possible interaction or merger event. A tail-like protrusion extends from the galaxy, which may be tidal debris resulting from a gravitational disturbance. The galaxy appears to be relatively smooth overall, but the tail suggests significant underlying dynamism.
