The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth, centrally concentrated luminosity profile with a subtle fading towards the outer edges. The core region shows a reddish hue, possibly indicative of an older stellar population, while the broader region has a slightly bluer color. The overall form is somewhat elongated, suggesting a deviation from a perfect spherical shape. There is no clear indication of spiral arms or a distinct disk component. No major signs of interaction with other galaxies, nor any prominent tidal tails or disturbances are observed.
