The galaxy appears to be a spiral, possibly of type Sa or Sb, observed at a significant inclination. A bright central bulge dominates the galaxy's luminosity, suggesting a substantial population of older stars. The bulge exhibits a smooth, featureless morphology. Faint spiral arms are visible extending from the bulge, though they are not well-defined and appear somewhat tightly wound. There appears to be relatively low star formation activity, suggested by the overall color of the disk being slightly yellow and lack of prominent blue star forming regions, except for a hint of faint bluish color in the outer arms on the left side. There's no indication of recent major merger activity or significant tidal distortions; it appears to be relatively undisturbed. Overall, the galaxy appears to be a fairly typical mid-mass spiral with a dominant bulge and modest levels of star formation.
