The galaxy appears to be an elliptical galaxy, or possibly a lenticular galaxy viewed at an oblique angle. It presents a smooth, diffuse light distribution. The galaxy exhibits an elongated shape, with the light intensity gradually decreasing from the center outwards. The core region displays a bright, concentrated glow, suggesting a dense stellar population or perhaps an active galactic nucleus. The color profile shifts subtly from yellowish-orange in the central bulge to a slightly bluer hue in the outer regions, although the overall color is predominantly redder. There appears to be little evidence of significant dust lanes or spiral arm structures within the galaxy. There may be very slight disturbances to the upper right suggesting minor interactions with an outside source. Based on the color and morphology, the galaxy is likely comprised mostly of older stars with a low rate of ongoing star formation.
