The galaxy appears as a single, relatively smooth object. The light profile suggests an elliptical morphology. The core is a bright, concentrated orange-yellow, indicating an older stellar population, potentially dominated by red giant stars. This central region smoothly transitions to a diffuse, fainter halo. The halo exhibits a slightly more reddish hue, though its color is difficult to distinguish due to its faintness. There are no apparent spiral arms, dust lanes, or other distinct features associated with disk galaxies. There is no evidence of tidal disturbances or interactions with other galaxies. Overall, the galaxy presents a relaxed, undisturbed appearance.
