The galaxy appears to be a late-type spiral, possibly of the Sc or Sd classification, seen edge-on. A prominent, elongated central bulge is visible, exhibiting a yellowish-orange hue, indicative of an older stellar population. The disk is oriented nearly perpendicular to the line of sight, with faint, blueish regions suggesting the presence of younger stars and ongoing star formation, especially on one side. The overall structure is elongated, with an approximate diameter of 6 kpc. Although there is some evidence of internal structure, there is no visual disturbance that would indicate a major merger event. The central bulge dominates the overall light output.
