The galaxy presents a generally smooth, elliptical appearance. The central region exhibits a high concentration of light, appearing as a bright, somewhat diffused core. The light gradually fades outward from the core toward the edges of the galaxy. Overall it displays a nearly round shape, with only the slightest elongation. There is little indication of spiral arms or other distinct structural features; the light distribution is relatively homogenous. Faint blue tinges are observed in the outer regions of the galaxy. There is no strong evidence of active galactic nucleus activity. A faint disturbance might be present, but it is not indicative of ongoing major merger events.
