The galaxy appears as a centrally concentrated object with a largely smooth morphology. The light distribution suggests a spheroidal shape, though it is not perfectly circular. There is a gradual decrease in luminosity from the center outwards, lacking any distinct spiral arms or prominent features. The color profile indicates a population of older stars, given the yellow-red hue dominating the galaxy's overall appearance. There might be minor disturbances or interactions evident in the galaxy's structure, as indicated by the slight irregularities in the outer regions.
