The object appears to be a lenticular or edge-on spiral galaxy. Its morphology is elongated and cigar-shaped, with a central bulge exhibiting a yellowish hue. The galaxy displays a smooth overall appearance. There is a distinct but smaller, bluish region offset from the central bulge, suggesting a region of active star formation. The majority of light is concentrated in the bulge, indicating an older stellar population within that region. There are slight indications of minor disturbance in the galaxy structure but no evidence of major disruption or a merger event. The galaxy shows a relatively high star formation rate.
