This galaxy exhibits a notable elongated morphology, appearing cigar-shaped. The central bulge presents a smooth, concentrated luminosity, suggesting a significant population of older stars. The disk component is also fairly smooth with subtle indications of spiral structure, though not sharply defined. The overall color profile suggests moderate star formation activity with the spiral arms appearing slightly bluer than the bulge. There is no immediately obvious evidence of a major ongoing merger, however, a slight irregularity in the shape and texture of the disk could indicate minor tidal interactions or recent accretion events.
