The galaxy presents as a spiral type, observed at a nearly face-on orientation. Two distinct spiral arms emerge from a central bulge, winding moderately. The arms appear somewhat tightly wound near the center and more open in the outer regions. The central bulge exhibits a moderate size, with a high concentration of light, suggesting an older stellar population, while the spiral arms show bluer hues, indicative of ongoing star formation regions. There's no evidence of a prominent bar structure within the central region. No signs of major mergers or significant tidal disturbances are observed in the surrounding structure, though some minor irregularities may be present.
