This galaxy appears to be an elliptical galaxy, exhibiting a largely smooth, symmetrical structure. The light is concentrated towards the center, with a gradual decrease in intensity outward. The color profile shows a generally yellow hue, suggestive of an older stellar population. The overall shape is round, with no obvious signs of spiral arms, bars, or significant dust lanes. There is no indication of ongoing major mergers or tidal disturbances. The galaxy likely has a substantial mass and is undergoing relatively low rates of star formation.
