The galaxy presents a moderately smooth morphology with some discernible features. It appears largely elliptical in shape, with a slight elongation, but not markedly cigar-shaped. There is a concentration of light towards the center, suggesting a bulge. The light distribution from the core outwards is gradual and diffuse, exhibiting a lack of distinct spiral arm structures. The overall color suggests a moderate population of older stars, with potentially a lower rate of ongoing star formation. There are hints of minor disturbances to the overall structure that may be the results of smaller mergers.