The galaxy presents as a lenticular or edge-on spiral, with a smooth, elongated profile. The central bulge is prominent and appears yellowish, indicative of an older stellar population. There is some indication of a faint, blueish disk extending beyond the bulge, suggesting some ongoing star formation, though seemingly at a lower rate. The galaxy's overall structure appears relatively undisturbed, lacking strong evidence of recent major merger activity. However, there might be minor disturbances or irregularities in the outer regions, warranting further investigation. The colour gradient from the central bulge to the outer disk supports the notion of a decreasing age of stellar populations towards the periphery. The galaxy's light profile is fairly smooth, hinting at a well-mixed stellar population and a lack of prominent star-forming regions.
