The galaxy presents as a somewhat elongated, cigar-shaped object. It exhibits a smooth overall appearance, although there is evidence of some internal structure, possibly a disk-like component. The color gradient transitions from a central yellowish-white core to a more reddish-orange periphery, suggesting a centrally concentrated older stellar population and potentially ongoing or recent star formation in the outer regions. There appears to be minor interaction or tidal disturbance visible, hinting at a possible recent or ongoing merger event. Overall, it seems to be a massive galaxy, with a moderate star-formation rate.
