The galaxy appears to be an elliptical type, presenting a largely smooth and concentrated light profile. The core region exhibits a bright, yellowish-orange hue, indicative of an older stellar population dominated by evolved stars. The galaxy appears to have a regular shape with a notable absence of spiral arms or a distinct disk. The light intensity decreases gradually from the center outwards, forming a relatively well-defined halo. There is a subtle color gradient suggesting that younger stars may be present in the outer regions, although this is difficult to ascertain given the smooth appearance. Minor disturbances in morphology are potentially observed, which could be indicative of recent or ongoing interactions with other galaxies.
