The galaxy presents as a spiral type, likely a disk galaxy viewed at a moderate inclination. There is a defined central bulge which appears bright and yellowish, indicating an older stellar population. Fainter spiral arms can be seen extending from the central bulge. These spiral arms appear to be loosely wound, suggesting a flocculent spiral structure. The disk component shows a somewhat clumpy structure in the spiral arms, possibly regions of active star formation. The overall color of the disk is bluer compared to the central bulge, further supporting ongoing star formation. There is no obvious evidence of tidal tails or morphological disturbances, suggesting that the galaxy has not recently experienced a major merger event. Based on the color and arm structure, this galaxy seems to be a relatively massive spiral galaxy, exhibiting moderate star formation activity.
