The galaxy exhibits a generally smooth, elliptical morphology. The light is concentrated toward the center, showing a bright, well-defined core. Moving outward from the core, the light decreases gradually without any distinct features such as spiral arms or a prominent disk. The galaxy appears to be primarily composed of older stellar populations, indicated by its yellow to reddish hue. There may be evidence of a slight tidal tail or faint stream of stars extending from the galaxy, but it appears very faint, or could be an artifact. There is no substantial evidence of significant ongoing star formation. No clear signs of a major ongoing merger are visible, though the possibility of past interactions or minor disturbances cannot be ruled out.
