The galaxy presents as a cigar-shaped structure, suggesting an elliptical morphology. The light distribution appears relatively smooth, with a gradual decrease in brightness from the central region outward. A hint of bluer tones is noticeable, particularly in what may be faint, diffuse outer regions or possibly areas of recent star formation within the galaxy, although this is not definitively pronounced. Overall, the galaxy exhibits features consistent with a relatively evolved system, but with the subtle potential for some ongoing star formation. The lack of prominent dust lanes or spiral arm structures further reinforces an elliptical classification. No obvious signs of major mergers are apparent, though subtle tidal features cannot be entirely ruled out.
