This galaxy presents as a somewhat face-on spiral, exhibiting a bright, concentrated central bulge region. The spiral arms are not sharply defined; instead, they appear somewhat diffuse and flocculent, possibly indicating a lower rate of star formation or a higher degree of dust obscuration. The overall color profile suggests a mix of stellar populations, with a yellower hue in the central regions potentially indicating older stars, and bluer tints in the outer regions that could be due to ongoing star formation. There's a slight asymmetry in the outer disk, possibly hinting at past interactions or minor disturbances, though no significant tidal features are readily apparent.
