This galaxy appears to be a relatively smooth, elliptical galaxy. The central bulge is prominent and generally spherical. The light is concentrated in the center, with the surface brightness decreasing gradually towards the outer edges. There are no obvious spiral arm structures or dust lanes visible. The galaxy presents a yellowish hue, suggesting an older stellar population with a lower rate of ongoing star formation. There may be very faint indications of some minor disturbances, but the overall structure is well-defined and undisturbed. It appears to be an isolated galaxy, without any major signs of an ongoing merger or interaction with another galaxy.
