The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. The core of the galaxy exhibits a bright, reddish-orange hue, suggesting a population of older, redder stars. Moving outwards from the core, the light fades gradually, and the color shifts towards a slightly greener tint, possibly indicating the presence of a younger stellar population or a small amount of star formation. The overall shape of the galaxy is approximately elliptical, with a slight elongation along one axis. There is no clear evidence of spiral arms or a prominent disk structure. Faint disturbances in the surrounding halo region, however, suggest the possibility of past minor merger events or tidal interactions, even though the central galaxy is not highly disturbed. The galaxy is overall a very smooth system with no high levels of current star formation.
