This galaxy appears to be an elliptical type with a relatively smooth morphology. The central region exhibits a high degree of luminosity, suggesting a concentrated nucleus, potentially hosting an active galactic nucleus or a supermassive black hole with ongoing accretion.

Moving outwards from the core, the galaxy displays a diffuse halo. There is a slight asymmetry to the overall shape, possibly indicating tidal interactions with another galaxy or recent merger activity. The outer regions show a more irregular distribution of light, with faint streams or plumes of material visible. This could be evidence of past or ongoing gravitational disturbances. 

The color distribution indicates the presence of multiple stellar populations. The central region appears bluer, suggesting the presence of younger, hotter stars or a higher rate of star formation. The outer halo shows a redder hue, possibly indicating an older stellar population. Evidence of minor disturbances can be noted on the sides of the central region, but the galaxy looks mostly uniform and round.
