The galaxy presents as a singular, relatively smooth object. Its morphology is elliptical, exhibiting a high degree of roundness. There is a concentration of light towards the center, suggesting a prominent galactic nucleus. The overall color profile appears to be redder, possibly indicating an older stellar population. The light is somewhat fuzzy, implying it is a significant distance from the observer. There is no apparent evidence of spiral arms or bar structure. No signs of major mergers are visible. The galaxy exhibits a generally undisturbed structure.
