The galaxy presents as a spiral type, viewed at a slight angle but approaching face-on orientation. A prominent central bulge exhibits a yellowish-white hue, indicating a significant population of older stars. Faint spiral arms extend outwards from the bulge, appearing tightly wound. These arms are bluer in color compared to the bulge, suggesting the presence of younger, hotter stars and ongoing star formation. The galactic disk, in general, appears smooth with an apparent lack of distinct star-forming regions. Based on its morphology, it appears to be in a relatively quiescent state with only a few signs of past or current interactions.
