The galaxy presents an elliptical morphology, displaying a relatively smooth, diffuse light distribution. A central bulge is visible, appearing more compact and brighter than the outer regions. The galaxy's color profile exhibits a somewhat bluer hue near the central region, suggesting the presence of younger stellar populations. The disk of the galaxy has some minor disturbances, perhaps indicating it is undergoing a minor merger. The galaxy is observed with a slight tilt relative to our line of sight. A faint, extended halo surrounds the central body of the galaxy.
