The galaxy presents a distinct spiral morphology. The spiral arms are well-defined and exhibit a relatively tight winding pattern around the central bulge. The bulge itself appears moderately sized, contributing significantly to the overall luminosity of the galaxy. The disk is clearly visible and oriented close to face-on. Although there is no apparent central bar, the lack of a bar could be down to resolution limitations. There is little evidence of any major merger events or significant tidal disturbances, however there is evidence of some features in the spiral arms. These feautures could be due to mergers, interactions with other galaxies, or just from star formation. The galaxy shows color variation, with a bluer color in the spiral arms possibly indicating active star formation. The color near the center is more reddish, possibly signifying an older stellar population.
