The galaxy appears to be a relatively compact object with an overall elliptical morphology. There is a noticeable color gradient, with a bluer core transitioning to redder hues in the outer regions. The core region exhibits a high degree of smoothness, suggesting an older stellar population. There is also a possibility of a faint disk-like structure. A faint arm-like structure is slightly visible, but this could also be due to distortion via a merger. The overall light distribution suggests the possibility of a merger event, although this may be subtle. Based on the asymmetry and disturbances, there's evidence of a possible ongoing interaction with a smaller galaxy, or remnants from a previous one.
