The galaxy appears to be a lenticular or early-type spiral galaxy, viewed at a significant inclination. The central bulge exhibits a high degree of smoothness and is elongated in shape. Evidence of a faint, diffuse disk is present, extending beyond the central bulge. The disk material appears relatively smooth with no obvious spiral arm structure visible in the image, but there is some color variation with the presence of some yellow/red regions toward the outer parts of the disk that could be evidence of older stars or dust lanes. The galaxy is elongated, with the major axis significantly longer than the minor axis. There is no evidence of any major mergers or significant tidal disturbances impacting the galaxy's overall morphology, but there could be a small disturbance.
