The galaxy presents as a spiral galaxy, with a noticeable central bulge. The bulge appears to be composed of older stars, indicated by its yellowish hue. The disk of the galaxy appears to be relatively smooth, with only hints of spiral arm structure. There is a subtle gradient in color from the center outwards, with the outer regions showing a slight blueish tint. This suggests a younger stellar population within the spiral arms and disk, where star formation may be ongoing. The galaxy's overall shape appears to be lenticular, suggesting it is an intermediate type between elliptical and spiral galaxies. No signs of significant ongoing mergers are visible, but a slight irregularity in the disk shape could indicate a previous minor interaction.
