The galaxy appears to be a spiral galaxy with a prominent, moderately sized bulge. The bulge exhibits a yellowish hue, indicative of an older stellar population. Faint, loosely wound spiral arms extend from the bulge, displaying a bluer color suggestive of ongoing star formation. These arms are somewhat patchy, with regions of higher luminosity possibly indicating areas of increased star-forming activity. There may be minor disturbances, as some of the spiral arm structures do not appear entirely regular. The galaxy doesn’t appear to be perfectly face on, but is presented at slight angle. There is no evidence of a strong bar structure. Overall, the galaxy is not overly smooth and has disk-like qualities.
