The galaxy appears to be a relatively smooth, elongated elliptical galaxy. The central region exhibits a high surface brightness and a yellowish-white color, suggesting a population of older stars. The light gradually fades outwards into the surrounding halo. The galaxy displays an intermediate ellipticity, appearing neither perfectly spherical nor highly flattened, with subtle hints of a disk shape that may contain some more complex features. There is no obvious presence of spiral arms or dust lanes. No significant morphological disturbances are apparent, indicating that the galaxy is likely isolated and not currently undergoing a major merger event. There may be a faint tidal tail or some minor asymmetry on one side of the galaxy, but there is no clear evidence of a major interaction.
