The galaxy presents as a face-on spiral, exhibiting a relatively compact morphology. A prominent central bulge is visible, appearing somewhat diffuse and dominating the overall luminosity. Faint spiral arms extend outward from the central region, showing a tightly wound structure. These arms display a mottled texture, possibly indicative of star-forming regions. There appears to be no bar structure. Overall, the galaxy exhibits a moderately inclined disk, lacking any major distortions or signs of mergers. The color profile suggests a relatively evolved stellar population, especially within the bulge.
