The galaxy presents as a relatively face-on spiral galaxy. A bright, concentrated central bulge is visible, exhibiting a yellowish hue. Surrounding the bulge, loosely defined spiral arms extend outwards. These arms display a mottled texture with areas of bluer light, suggestive of recent star formation regions interspersed with older stellar populations. The overall shape of the disk is elliptical, appearing slightly elongated. There is no obvious evidence of major tidal disturbances or recent merger events. The spiral arms exhibit a moderate degree of winding, neither tightly wound nor particularly loose. A faint bar-like structure might be present, but the resolution is not sufficient to confirm its presence or strength conclusively. The dust lanes are difficult to observe but seem to be relatively minimal due to the face-on orientation.