The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentration of light towards its center, suggesting a prominent galactic nucleus. It appears mostly featureless, lacking defined spiral arms or significant dust lanes. Its shape is more akin to a rounded form, with a slight elongation that does not appear to be a cigar shape. There are no major signs of merging or significant disturbances, indicating that the galaxy is most likely in a relatively stable state.

The galaxy's color appears yellowish to orange, suggesting an older stellar population, with lower levels of ongoing star formation. The overall light distribution is fairly smooth and does not show significant clumping of stars or HII regions that are usually signs of star formation.
