The galaxy appears to be a lenticular or early-type spiral galaxy viewed at a moderate inclination angle. Its overall shape is elongated, with the major axis significantly longer than the minor axis. The central region exhibits a bright, relatively smooth bulge, indicating a high concentration of stars. The light profile appears smooth and centrally concentrated, with a gradual fading towards the outer edges. There is some evidence of a disk-like structure, with subtle color variations, which might be faint spiral arm segments. The dominant color is yellowish-white, with hints of bluer regions in the outer disk, suggesting the presence of younger stellar populations, although star formation appears subdued. No significant dust lanes or prominent star-forming regions are readily apparent. The overall impression is of a galaxy transitioning from a spiral to an elliptical morphology. Evidence indicates that there are no major mergers disturbing this object. 
