The galaxy presents as a spiral, viewed at a slight angle but not completely edge-on. The disk exhibits some visible structure, suggestive of spiral arms, though they are not sharply defined. The overall color profile indicates a population of both older, redder stars, particularly concentrated in the central bulge, and younger, bluer stars within the disk. A moderate bulge appears present. There is no strong bar structure visible. No major merger events are immediately apparent, though some minor disturbance is difficult to rule out. 
