The galaxy presents a distinct spiral morphology. Two prominent arms originate near the central bulge, appearing somewhat tightly wound. The bulge itself is moderately sized, exhibiting a yellowish hue suggestive of an older stellar population. The spiral arms display a bluer color, indicative of active star formation. There appears to be minimal evidence of strong bar structures or major mergers; however, a slight asymmetry in one of the arms may suggest minor gravitational interactions, such as tidal distortions from a past or ongoing minor merger event. The disk is viewed at a slight angle, providing a partial view of the overall structure. There is some evidence of dust lanes within the spiral arms, appearing as slightly darker regions against the blue light.
