The galaxy appears to be a relatively smooth, elliptical galaxy with an apparent red shift. The central bulge is luminous, indicating a high concentration of older stars. The galaxy displays a yellow-orange hue that decreases in intensity from the center to the outer edges. The galaxy appears slightly oblong in shape, and it shows no apparent signs of spiral arms or significant dust lanes. There are no obvious signs of active galactic nuclei or recent major mergers, although there appears to be minor disturbances. The observed color suggests a moderate level of ongoing star formation, with the presence of both young, hot stars and older stellar populations contributing to the overall spectral energy distribution.