The galaxy presents a lenticular, disk-like morphology with a prominent central bulge. The disk appears to be inclined at a moderate angle relative to our line of sight, though is potentially approaching edge-on. The bulge exhibits a smooth, concentrated appearance, suggesting an older stellar population. Evidence of spiral arm structure is present. The color gradient transitions from a bluer hue in the disk to a redder one in the bulge. The disk exhibits clumpy features along its plane, potentially indicating star-forming regions. Overall, the galaxy appears relatively undisturbed, exhibiting no signs of ongoing major mergers, though some minor asymmetry/disturbance is apparent in the outer regions of the disk.
