The galaxy presents as a relatively compact, yellowish-orange structure. Its morphology appears to be primarily smooth, lacking strong spiral arm features or a prominent central bulge. The galaxy shows a moderately elliptical shape, closer to in between round and cigar shaped with an estimated effective radius of about 4 kiloparsecs. Some minor disturbances are visible in the galaxy's structure, possibly indicating recent or ongoing interactions or internal dynamics. The absence of strong blue color suggests relatively low ongoing star formation. Overall the galaxy's light is consistent with an older stellar population and it appears relatively massive.
