The galaxy presents as a spiral type, with a moderately defined structure. The arms are visible and somewhat patchy, indicating areas of both active star formation and dust obscuration. The arms have a fairly disorganized appearance and extend out from the central bulge.

The central bulge is significant, contributing substantially to the overall luminosity of the galaxy.

There appears to be some distortion or asymmetry in the overall shape, possibly indicating an ongoing or past interaction with another galaxy. This is evidenced by a slight warp or irregularity in the disk structure. There are areas in the outer spiral arms of the galaxy that could be the effects of minor merging, and potentially signs of tidal features. 

The color profile suggests the presence of both younger, bluer stellar populations in the spiral arms and older, redder populations in the bulge. The galaxy exhibits a mixed population of stars and appears to be in a transitional phase of its evolution.
