The galaxy exhibits a primarily smooth morphology, with a slight elongation along a major axis. The color gradient suggests a relatively older stellar population throughout the galaxy, as indicated by the redder hues, particularly in the outer regions. The central region of the galaxy appears bright and compact. The overall light distribution suggests minimal disk features. There is no obvious evidence of ongoing major merging events or significant tidal disturbances. However, subtle asymmetry in the light distribution may indicate minor interactions or internal dynamical processes.
