The galaxy presents as a spiral type, displaying a prominent disk structure. The disk is oriented at an angle relative to our line of sight. Evident spiral arms are visible, wound relatively tightly around a central bulge. The bulge appears moderately sized. There is strong suggestion of a bar structure bisecting the bulge along its major axis. The galaxy exhibits subtle signs of tidal disruption or past interaction, with a slight asymmetry in the spiral arm distribution. The spiral arms are characterized by a flocculent morphology with what seem to be areas of active star formation. The color profile across the galaxy displays a gradient, with the bulge appearing more yellow-red suggestive of older stellar populations, while the spiral arms exhibit a bluer hue, indicative of younger, hotter stars.
