The galaxy appears to be an elliptical, exhibiting a smooth, mostly featureless morphology. Its overall shape is consistently round. There appears to be no evidence of spiral arm structure or a prominent disk. The color profile indicates the presence of older stellar populations, with a yellowish-orange hue dominating the galaxy's central regions. A slight gradient in color intensity can be observed, with a brighter, more concentrated core fading into a fainter outer halo. There is no apparent signs of any major tidal distortions, ongoing mergers, or significant dust lanes within the galaxy's visible structure. The galaxy appears as a well-defined, isolated system.
