The galaxy presents a predominantly smooth morphology, suggesting it is likely an elliptical or lenticular type. There is little evidence of spiral arms or significant dust lanes. The galaxy exhibits an elongated, cigar-like shape, being much longer than it is wide. The light distribution appears relatively even across the galaxy, with a concentration toward the central region but lacking a bright, well-defined nucleus. The overall color is somewhat blue-white, which could indicate a component of young stars, although the smoothness of the morphology suggests that the galaxy's star formation rate is low. There is some indication of minor asymmetry or a subtle distortion in its shape, possibly suggesting past interactions with a smaller companion galaxy. The galaxy does not appear to be undergoing any major merger activity and shows no signs of tidal tails or strong disturbances.
