The galaxy appears to be a single, relatively smooth object. Its overall morphology is elliptical, although it is not perfectly circular, exhibiting a slight elongation. There is no defined spiral structure or bar visible. The galaxy displays a color gradient, with the central regions appearing more reddish and the outer regions gradually becoming bluer. This could indicate a difference in stellar populations, with older, redder stars concentrated in the core and younger, bluer stars in the outer regions. I don't observe any signs of major ongoing mergers or strong tidal interactions. However, there is a hint of minor asymmetry or irregularity in its outer regions, which could be indicative of a past minor merger or disturbance. The galaxy appears well-defined and compact.
