The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be largely featureless, lacking well-defined spiral arms or a prominent bar. The central region of the galaxy exhibits a bright, concentrated core, suggestive of a significant stellar population or possible active galactic nucleus activity. Moving outwards from the core, the luminosity gradually decreases, forming a more diffuse halo. The shape of the galaxy appears to be somewhat elongated. There is a subtle color gradient, with the core displaying a more yellow-red hue, potentially indicating an older stellar population. The outer regions appear slightly bluer, suggesting the presence of younger stars, however these colors may also be because of redshift. There are no signs of any ongoing major merging events, although a slight disturbance might be present.
