The galaxy presents as an elongated structure with a noticeable bulge. The central region exhibits a smooth, diffuse appearance, which transitions into a less defined disc. The galaxy’s color appears yellow-orange, suggesting an older stellar population and relatively low star formation rate. There is some evidence of asymmetry in the structure, specifically a slight irregularity along one edge of the disc, possibly indicating a minor gravitational interaction or disturbance. No distinct spiral arm structures are readily discernible. Overall, the galaxy appears to be an elliptical type, likely with moderate mass.
