The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light profile suggests a gradual decrease in intensity from the core outwards. There is no readily apparent disk structure or spiral arm features. The galaxy appears nearly circular in shape. There's a hint of redder hues within the central region, potentially indicating an older stellar population. The outskirts are fuzzier, possibly indicating a lower density of stars, or the effects of image resolution at this distance. There is no evidence of active galactic nuclei (AGN) activity or strong star formation from visual inspection. No obvious tidal features or signs of interaction with another galaxy are visible.
