The galaxy exhibits a generally elliptical morphology, appearing largely smooth in its central regions with a bright, concentrated nucleus. Fainter, diffuse spiral arms extend from the central bulge. The color profile suggests the presence of both older stellar populations in the bulge, indicated by the yellow hue, and younger stellar populations within the arms, showing a faint bluish tint. The overall shape displays a slight flattening, suggesting the galaxy is viewed at an angle, but not completely edge-on. There may be some evidence of minor tidal disturbances or ongoing merging activity, with some asymmetry observed in the distribution of light in the outer disk.