The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is little evidence of spiral arms or significant disk features. The color gradient appears to transition from a yellowish core to a slightly redder outer halo, suggesting an older stellar population dominating the galaxy's composition. The overall morphology indicates a system approaching quiescence, with low levels of on-going star formation. No tidal tails or major disturbances are visible, indicating that the galaxy is likely not undergoing any major mergers. The galaxy exhibits a somewhat in between roundness, with very little cigar shaping. 
