The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile, with the brightest region located in the core. The light gradually diffuses outwards from the center, with no distinct spiral arm features or a prominent disk visible in the image. 

There is a slight color gradient, with a subtle bluish hue noticeable in the outer regions of the galaxy. This suggests the presence of a younger stellar population in these areas. The main body of the galaxy appears more yellowish, which would be consistent with an older population of stars.

The galaxy's overall shape is close to round, without any obvious signs of significant tidal disturbances or interactions with neighboring galaxies. There is no clear evidence of any major ongoing mergers or disruptions to its structure. It looks to be a fairly isolated system, evolving in a relatively undisturbed environment.
