The galaxy appears to be a spiral galaxy, viewed at an oblique angle, but not completely edge-on. A central bulge is clearly visible, exhibiting a yellowish-white color, suggesting a population of older stars. Faint spiral arms can be discerned extending from the central bulge. These arms are somewhat diffuse and not sharply defined. The arms appear bluish, indicating the presence of younger, hotter stars and ongoing star formation. The dust lanes are not clearly observed. The galaxy exhibits a moderate degree of internal structure, with hints of asymmetry in the spiral arm distribution. The galaxy doesn't appear to be undergoing any major merging activity, though the observed structure might indicate a minor gravitational interaction in the past.
