The galaxy presents as a spiral type, observed at a slight angle relative to edge-on. Its central bulge appears moderate in size and exhibits a yellowish hue, indicative of an older stellar population. Distinct spiral arms are visible, tracing outward from the core. The arms display a relatively consistent pitch angle and could be described as having medium winding. Two spiral arms are clearly visible. There is no evidence of significant tidal disturbances, with the galaxy appearing relatively undisturbed. Overall, it is an apparent spiral structure with moderate arms and a prominent bulge.
