The galaxy presents as an elongated, disk-like structure, suggesting an edge-on or highly inclined spiral or lenticular morphology. A prominent central bulge is evident, appearing bright and concentrated. The disk exhibits a relatively smooth texture overall, with some indication of underlying structure. The light distribution is dominated by yellow and red hues, which suggests an older stellar population. The overall color profile indicates a relatively low star formation rate. There are no obvious signs of tidal interactions or major disturbances in its morphology, suggesting a gravitationally settled system. 
