The galaxy presents as a relatively smooth, centrally concentrated object with a near-spherical morphology. It exhibits a color gradient, appearing redder toward its core and becoming slightly bluer in the outer regions. There is no discernible spiral structure or distinct features such as prominent dust lanes or star-forming regions. The overall appearance suggests a lack of significant ongoing star formation. Subtle signs of a possible minor disturbance are present, potentially indicating a previous or ongoing interaction with a smaller companion galaxy.
