The galaxy presents as a spiral type, exhibiting well-defined spiral arm structures. A substantial portion of the galaxy's light emanates from a bright central bulge. The spiral arms are relatively open and show a granular texture, suggesting active regions of star formation. A bar structure is present, though not particularly prominent, which extends through the central region of the galaxy. The color of the central bulge appears more yellow/red compared to the bluer hues of the spiral arms, indicating an older stellar population residing within the bulge. The outer regions of the galaxy appear less defined, possibly indicating the presence of a diffuse halo of stars and gas. No significant tidal disturbances or signs of a major merger event are apparent, although some minor asymmetries within the spiral arm structure could suggest past interactions. The overall morphology is that of a relatively undisturbed, late-type spiral galaxy with ongoing star formation.
