The galaxy presents a clear spiral structure, with two prominent arms emanating from a central bulge. These arms display a tightly wound morphology, suggesting a relatively high rate of rotation. The arms are somewhat flocculent, with regions of enhanced luminosity indicating possible active star formation. The color gradient suggests a higher concentration of older stars towards the center. The galaxy does not appear to be undergoing a major merging event but exhibits minor disturbances that could be indicative of an interaction or recent accretion event. The central bulge appears relatively small compared to the overall disk size, classifying it as a late-type spiral galaxy.
