The galaxy presents an elliptical morphology, appearing relatively smooth and featureless. Its shape is somewhat elongated, exhibiting a cigar-like appearance. The central bulge is prominent, displaying a yellowish-orange hue. The outer regions of the galaxy appear bluer, suggesting the presence of younger stellar populations. There is a subtle indication of a faint disk structure, although it is not a dominant feature. There is no apparent evidence of any major ongoing merger activity or significant tidal disturbances, although some minor irregularity cannot be ruled out. Overall, the galaxy appears to be a relatively evolved system with evidence of past star formation that may still be active.
