The galaxy presents as a lenticular or possibly an edge-on spiral morphology. A bright, seemingly spheroidal central bulge dominates the overall luminosity. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. A faint, flattened disk is visible extending from the bulge. The disk appears relatively smooth, lacking any prominent spiral arm structures or distinct dust lanes. The galaxy displays a noticeable elongation, indicating a significant inclination relative to our line of sight, making it difficult to discern detailed features within the disk. The outer regions of the disk gradually fade into the background, lacking a sharp, well-defined boundary. No obvious signs of recent major merger events are apparent.
