The galaxy presents as a somewhat elongated, disk-like structure. It appears relatively smooth in overall texture, with a dominant central bulge that seems less prominent at the edges. There is a hint of spiral arm structure, though indistinct. The light distribution suggests active star formation; bluer hues along the disk suggest ongoing formation, whereas yellower regions in the bulge may be from an older stellar population. There are indications of some minor disturbances, perhaps evidence of past interactions with smaller galaxies, or mergers. The galaxy exhibits properties suggesting an intermediate-mass system, currently with a relatively low star formation rate. The morphology suggests an intermediate stage between a pure elliptical and a fully developed spiral galaxy.
