This galaxy presents as a relatively smooth object with an elliptical morphology. The central region exhibits a bright, concentrated luminosity, suggesting a prominent galactic nucleus. The light distribution gradually decreases toward the outer regions, lacking any discernible spiral arm structures or bar features.

There are subtle color gradients visible, with the central region appearing more yellow-white, potentially indicating an older stellar population. The outer edges display a slight red hue, which could be attributed to dust extinction or a younger, redder stellar population on the outskirts, but it is only subtle.

The overall texture of the galaxy appears homogenous, without any significant irregularities or signs of ongoing major mergers. There are no tidal tails or other visible indications of recent gravitational interactions. There seems to be a possible minor disturbance in the disk, but it could be difficult to tell if it is a true disturbance. The relatively smooth appearance suggests a well-evolved system that is in a fairly stable state.
