The galaxy appears as a moderately bright, yellowish-white object. Its morphology is largely smooth and spheroidal, with no readily apparent spiral arm structures or a prominent disk. The overall shape approximates a rounded, elliptical form, showing minimal elongation. There may be some minor visual disturbances, however this may be blending with background objects. There is no clear evidence of a recent major merger or significant tidal interactions, nor is there evidence for a major dust lane obscuring the galactic nucleus. The color suggests a relatively evolved stellar population, although there might be a small amount of ongoing star formation contributing to the overall luminosity. The galaxy appears relatively isolated within its immediate surroundings.
