The galaxy presents a largely smooth and rounded morphology, appearing elliptical in shape. The light distribution shows a central concentration that is bright and yellowish, suggesting an older stellar population dominates the core. Fainter, bluer light extends outwards from the center, possibly indicating the presence of younger, star-forming regions in the outer parts of the galaxy, but this is minimal. There is no clear evidence of spiral arms or a prominent disk structure. No significant signs of tidal disturbances, mergers, or other major interactions are visible, although there may be minor disturbances.
