The galaxy presents an elliptical morphology, exhibiting a smooth, diffuse light distribution that diminishes gradually from its center. The core region appears brighter and has a slightly redder hue, potentially indicating an older stellar population. Moving outwards from the core, the galaxy's color shifts subtly towards bluer tones, hinting at the presence of younger stars or regions of ongoing star formation, although this activity is relatively subdued. The overall shape is elongated with a relatively high degree of symmetry, and there are no obvious signs of spiral arms, bars, or significant dust lanes, supporting the classification as an elliptical galaxy. There is also a very slight possibility of a minor disturbance in the gravitational field.
