The galaxy exhibits a prominent spiral structure. Two distinct spiral arms originate from the central bulge and extend outwards. The arms display a fairly consistent pitch angle indicating a winding pattern. The arms are well defined and appear to be active regions of star formation, judging by their irregular texture and varying color. The central bulge of the galaxy appears moderate in size, contributing to the overall structure of the galaxy without dominating it. There appears to be some disturbance in the shape, possible hinting at an interaction or recent merger with a smaller system, or possibly minor internal instabilities. The galaxy's disk is oriented at a moderate inclination angle relative to our line of sight.
