This galaxy presents as a spiral with a notable disk structure. The spiral arms are well-defined, appearing relatively tightly wound around a central bulge. Two primary arms can be traced, with the potential for bifurcations or less distinct arm segments. The bulge exhibits a moderate size relative to the overall galactic disk. The dust lanes within the spiral arms are visible, contributing to the patchy appearance of the arms. The galaxy exhibits a degree of asymmetry, possibly indicative of past or ongoing gravitational interactions, or internal dynamic processes affecting its structure. Evidence of active star formation regions exist, as indicated by brighter, bluer knots along the spiral arms, although these regions do not dominate the galaxy's overall luminosity. The central bulge appears comparatively smooth and featureless in contrast.
