The galaxy presents a lenticular or possibly a spiral morphology, observed at a moderate inclination. It displays a central bulge that appears relatively smooth and featureless, indicating an older stellar population. The disk component exhibits a faint, blueish tint, suggestive of ongoing, albeit low, levels of star formation. There appears to be a minor interaction or disturbance visible in the disk, possibly a tidal feature or an indication of a minor merger event. The overall color of the galaxy suggests that it is undergoing a relatively quiescent phase of star formation, with a mass within the range typical of average-sized galaxies. There is a suggestion of dust lanes or patchy obscuration within the disk, although the image resolution limits detailed analysis.
