The galaxy presents as a spiral galaxy with a prominent central bulge. The bulge region appears yellowish in color, indicative of an older stellar population. Fainter spiral arms extend outward from the central bulge. The arms display a bluer hue, suggesting more recent or ongoing star formation activity. The spiral arms are moderately wound. The galaxy appears to be in relative isolation, with no obvious signs of major tidal disturbances or ongoing mergers, although there may be minor irregularities in the arm structure that suggest past interactions. The disk is viewed at a moderate inclination, not quite face-on or edge-on. The overall morphology suggests a galaxy with a mixed stellar population and ongoing star formation.
