The galaxy presents an elliptical morphology, appearing as a spheroid with a smooth, diffuse light distribution. The color gradient transitions from a yellowish-white core to a bluer periphery. There is little evidence of spiral arm structure or distinct features, indicating it is likely a relatively evolved system. The shape is elongated, not perfectly spherical, suggesting a non-negligible rotational component or a recent minor merger. The lack of significant dust lanes or prominent star-forming regions reinforces the classification as a relatively quiescent galaxy.
