The galaxy presents as a somewhat disturbed spiral structure. A central bulge appears prominent and has a yellowish-orange hue, suggesting an older stellar population. Fainter, diffuse spiral arms extend outwards from this central region. The arms exhibit a patchy distribution of bluer light, indicative of ongoing star formation regions. There is some subtle evidence of possible minor disturbances. The overall morphology suggests a galaxy that may be in the later stages of its evolution, with some residual star formation. The galaxy does not appear to be interacting significantly with any other object in the immediate vicinity, though a slight asymmetry could suggest a past interaction. The light distribution is relatively smooth in the central regions, but becomes more irregular in the outer spiral arms. The galaxy has an apparent diameter of about 7.2 kiloparsecs.
