The galaxy appears relatively compact with a slightly elongated profile. It exhibits a generally smooth appearance with a faint, diffuse halo extending outwards. There is a subtle indication of spiral structure in the disk, with hints of arm-like features that do not show a well-defined morphology. There is little evidence of substantial dust lanes or bright star-forming regions within the galaxy. The galaxy's central region appears marginally brighter and more concentrated than the outer regions. Overall, the galaxy presents itself as a primarily unfeatured system, possibly an early-type spiral or lenticular galaxy with a fading disk. There is also an indication of a possible minor disturbance in the galaxy's morphology, such as a slight asymmetry or faint tidal feature, suggesting that the galaxy may have experienced or be currently undergoing a minor merger event.
