This galaxy presents a generally smooth morphology, appearing elliptical in shape with a notable elongation. It exhibits a strong central bulge, concentrated and bright, suggesting a high density of older stellar populations. The color profile indicates a redder core transitioning to slightly bluer hues in the outer regions. There's minimal evidence of prominent spiral arms or dust lanes, supporting the classification as an elliptical galaxy. The smooth, relatively featureless appearance suggests the galaxy is in a late stage of its evolution, with a relatively low star formation rate. The isophotes appear to be generally regular, with only minor irregularities observed, indicating it is likely undisturbed, without any major ongoing merging events.
