The galaxy presents a disk-like morphology, inclined relative to our line of sight. A prominent central bulge dominates the galaxy's core, exhibiting a smooth, concentrated luminosity profile. Fainter spiral arm structures extend outward from the central bulge, with indications of star formation. These arms appear somewhat tightly wound. There is a suggestion of a bar-like feature crossing the central bulge. The galaxy's color profile suggests a mix of stellar populations, with the bulge appearing yellower, indicative of older stars, and the arms possessing a bluer hue, likely due to the presence of younger, hotter stars. Overall, the galaxy does not appear to be undergoing any major mergers or significant tidal disturbances.
