The galaxy appears to be an intermediate spiral or a lenticular galaxy, exhibiting both smooth and featured characteristics. There seems to be a central bulge with an intermediate level of roundness. The galaxy does not show a well-defined spiral arm structure, but it exhibits some irregularity and possible tidal features, perhaps related to a prior minor interaction or merger event. Evidence of ongoing star formation is suggested by the patchy blue regions in the disk, although it is not strongly pronounced. Overall, the galaxy displays a mix of colors, with the central region showing a more yellow hue and the outer regions showing more blue, suggestive of differing stellar populations. The morphology suggests the galaxy is likely undergoing a period of transition, possibly due to the merging event(s), from a more regular spiral galaxy to a more disturbed elliptical type.
