The galaxy presents as a relatively smooth, elliptical morphology. The core appears to be quite bright and concentrated with a yellowish hue, indicating an older stellar population. The galaxy exhibits a gradual fading in luminosity from the center outwards, with no discernible spiral arm structures or significant dust lanes visible in this image. The shape is somewhat elongated, suggesting an elliptical galaxy that is not perfectly spherical but rather, more akin to an in-between round fraction, and cigar shaped fraction. There are no apparent signs of a major ongoing merger event, though minor disturbances cannot be ruled out based on this single image. The galaxy seems to be a relatively isolated system, without clear tidal tails or interactions with nearby companions that would be detectable in the available visual data. Overall, it presents as a fairly typical, well-evolved elliptical galaxy.
