The galaxy presents a generally smooth, elliptical morphology. The light distribution is concentrated towards the center, displaying a bright, yellowish core, indicative of an older stellar population. There is little evidence of spiral arms or distinct disk features. The shape is not perfectly spherical; it appears somewhat elongated. Fainter blue-ish hues can be observed extending from the central region, suggesting possible regions of younger star formation activity, though it appears minimal. There are no obvious signs of major disturbances such as tidal tails or prominent dust lanes that would strongly suggest a recent major merger event.
