The galaxy appears as a centrally concentrated object with a smooth morphology. Its overall shape is elliptical, exhibiting high roundness. The galaxy has a radial gradient in surface brightness, with a bright core that gradually fades into the outer regions. There are no discernible spiral arms, bars, or other distinct features typically associated with disk galaxies. The galaxy shows a relatively red color, suggesting an older stellar population. There is no indication of significant ongoing star formation or major disturbances in its structure, indicating a state of relative quiescence.
