The galaxy appears as a relatively compact, elliptical-like system. It presents a smooth, featureless morphology with no discernible spiral arm structure or prominent dust lanes evident in this image. The light distribution is centrally concentrated with a gradual falloff in surface brightness towards the outer edges. There are no signs of tidal tails or significant morphological disturbances, suggesting it is not currently undergoing a major merger. The color index shows a moderate red color suggesting an older stellar population with a suppressed rate of recent star formation. The overall roundness indicates a likely classification as an elliptical galaxy, possibly of type E3-E4.
