The galaxy exhibits a moderately bright central bulge that appears yellowish-white in color, indicating a population of older stars. A faint, relatively smooth disk surrounds the bulge. The disk appears slightly flattened. The overall morphology suggests a relatively early-type spiral galaxy, possibly an Sa or Sb, although the arms are not well-defined. There is a hint of blueish color within the outer disk, potentially indicating some regions of ongoing star formation. The galaxy appears fairly isolated with no obvious signs of recent major merger activity or significant tidal disturbance.
