The galaxy presents as a slightly inclined, elongated structure. There is a discernible bulge region that appears yellowish-orange, indicating a likely concentration of older stellar populations. The disk component is bluish-white, suggestive of younger stars and ongoing star formation. The galaxy's overall form appears relatively smooth, but with hints of potential disturbances or faint spiral arm structures extending from the bulge. The light distribution is generally concentrated towards the center, fading gradually into the outer regions of the galaxy.
