The galaxy appears as a moderately luminous, yellowish object. Its morphology is primarily smooth, with a slight elongation suggesting a shape somewhere between round and cigar-shaped. There is some subtle asymmetry to the distribution of light within the galaxy, but no clear evidence of spiral arms or a distinct disk structure. The color suggests a population of older stars, with relatively low ongoing star formation. There is no strong evidence of a major ongoing merger, although a minor disturbance or subtle interaction cannot be entirely ruled out based on the image alone. The galaxy is a relatively massive object, based on its apparent luminosity, which makes it closer to a larger galaxy.
