The galaxy appears to be an elliptical or lenticular type, with a largely smooth, symmetrical light distribution. The galaxy exhibits a concentration of light toward the center, gradually fading outwards. There is a slight elongation in shape, but it appears mostly rounded. There is no clear evidence of spiral arms or a prominent disk structure. The color gradient suggests an older stellar population, with a yellowish-orange hue more concentrated toward the core. There is minimal evidence of active star formation regions or significant dust lanes. The galaxy seems relatively isolated, with no obvious signs of major mergers or tidal disturbances, though some minor disturbance cannot be ruled out.