The galaxy presents as a spiral type, viewed at an oblique angle, but not quite edge-on. A prominent central bulge is observed, exhibiting a yellowish hue, likely indicating an older stellar population. Faint spiral arms appear to emanate from the central bulge, displaying a bluish tint, which may signify the presence of younger, hotter stars and ongoing star formation. Two main arms are visible. The arms are somewhat tightly wound. Overall, the galaxy appears to have a moderate luminosity, with the bulge contributing significantly to its total brightness. Some signs of a bar-like structure are also observed within the central region. There is no clear evidence of major disturbances or a recent merger event.
