The galaxy appears to be an elliptical galaxy, exhibiting a smooth, largely featureless morphology. Its shape is generally rounded, with a slight deviation from perfect circularity. The galaxy displays a radial brightness gradient, with a bright, concentrated core that gradually fades into the surrounding halo. The color is notably redder toward the center, suggestive of an older stellar population dominated by red giant stars. The outer regions show a bluer hue, hinting at a possible younger stellar population or the presence of some star formation, though this is subtle. There is no evidence of spiral arms, a prominent disk, or any significant dust lanes within the visible light. The overall appearance suggests a gravitationally relaxed system with limited ongoing star formation. No signs of any major mergers or tidal disturbances are apparent.
