The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its overall shape approximates a flattened spheroid with a high degree of roundness, with minimal apparent disturbance in its structure.

A pronounced central bulge, exhibiting a warmer color, dominates the galaxy's core. The bulge seems to gradually transition to a cooler, bluer hue at the galaxy's periphery, suggestive of differences in stellar populations.

There is minimal indication of spiral arm structure or prominent dust lanes. Faint features or subtle irregularities are visible in the outer regions, possibly hinting at weak tidal interactions or internal dynamics. However, there is a distinct lack of any major mergers.
