The galaxy presents as a relatively smooth, elliptical-like structure. Its core is luminous, with a yellowish hue indicating an older stellar population. The light appears consistent across the central region, lacking distinct features such as spiral arms or prominent dust lanes.

The outskirts of the galaxy show a gradual decrease in luminosity, fading into the background sky. The color shifts slightly toward redder tones towards the outer edges. There is no clear evidence of tidal tails or strong gravitational disturbances. The light appears to be evenly distributed. The galaxy is well-defined, and no signs of recent major mergers are observed. There may be a ring structure in the blue, however the resolution is not high enough to say definitively.
