The galaxy appears to be a relatively bright, lenticular or early-type spiral system, seen at an oblique angle. The central bulge is prominent and appears quite smooth with a high concentration of light. Moving outward from the bulge, a disk is observed, although the arms are not well defined. The galaxy has a fairly smooth overall appearance, with the disk presenting some mild disturbances but no strong evidence of major mergers or tidal interactions is visible. The galaxy exhibits a moderate degree of ellipticity. Color gradients suggest that the bulge is composed of older stellar populations, while the disk appears bluer, likely indicating ongoing or recent star formation, albeit at a low rate. Overall, the galaxy displays properties consistent with a system transitioning from spiral to elliptical morphology.
