The galaxy presents as a relatively smooth, elliptical-like structure with a subtle, elongated morphology. The overall color gradient suggests it is likely comprised of an older stellar population with a notable lack of substantial dust lanes. The blueish hue observed indicates a slight presence of more massive, young stars in the galaxy. However, the absence of well-defined spiral arms or intense star-forming regions further supports the classification of this galaxy as a possible lenticular or early-type spiral transitioning to a more elliptical form. There may be minor disturbances. The galaxy appears to have no central bulge, or it is not clearly visible at this resolution. Overall, the galaxy is a generally smooth object that is somewhere in between being round and cigar shaped.
