The galaxy presents as a primarily smooth object, with an intermediate level of roundness. There is a slight suggestion of disturbed morphology, potentially indicative of a minor interaction or merger. The light distribution appears centrally concentrated, with a gradual decline in surface brightness moving outwards. Color gradients are subtle, with a possibly slightly bluer core region surrounded by a redder halo. This suggests that the galaxy is likely an elliptical galaxy with a relatively old stellar population with a potential for minor recent star formation in its core.
