The galaxy presents a predominantly smooth morphology, with an elliptical appearance. The light profile suggests a centralized concentration, decreasing in intensity outwards. There is a slight elongation, not significantly deviating from a circular form.  The galaxy exhibits a color gradient, transitioning from a bluer hue in the central region to redder tones in the outer regions, possibly indicating differing stellar populations or dust distribution. There are no apparent spiral arms or significant disturbances to suggest any current major merger activity, although some minor interaction cannot be entirely ruled out. The galaxy appears relatively isolated within its immediate field.
