The galaxy presents a lenticular or early-type spiral morphology, with a dominant central bulge and a flattened disk. The bulge appears smooth and exhibits a redder color index, suggesting an older stellar population. The disk shows a bluer color index, indicating the presence of younger, hotter stars and possibly ongoing star formation. The galaxy's overall shape is elongated, hinting that we may be viewing it at a slight inclination. There may be some evidence of minor disturbances in the outer regions of the disk, as the light appears more irregular there, possibly caused by minor gravitational interactions. The size appears moderately large, with an estimated effective radius of a few kiloparsecs.
