The galaxy presents a spiral morphology, with two distinct spiral arms emanating from a central bulge. The arms exhibit a moderate winding, neither tightly wound nor loosely defined. These arms appear flocculent and are characterized by patchy regions of star formation, evidenced by the irregular distribution of bluer light, which indicates the presence of younger, hotter stars. The central bulge displays a more uniform, yellowish hue, which could be indicative of an older stellar population. A strong bar-like structure appears to be present across the central region of the galaxy, potentially influencing the spiral arm structure. There are no obvious signs of a major merger event, however there are minor disturbances that are visible in the arms that suggest minor interactions with other galaxies. Overall, this galaxy exhibits a relatively normal spiral structure with moderate star formation activity.
