The galaxy presents as a moderately inclined spiral, showing evidence of both a central bulge and a disk component. The bulge appears yellowish-orange, suggesting a population of older stars. The disk exhibits a mottled texture with hints of blueish regions, possibly indicating areas of ongoing star formation. The spiral arms are not well-defined but appear somewhat flocculent. The galaxy is not perfectly circular, displaying a slight elongation indicative of its inclination. There may be some minor disturbances in the disk, potentially suggesting a past or ongoing interaction with another galaxy, though no clear merging companion is visible in this image.
