The galaxy presents as a structure with a smooth, centrally concentrated morphology. There is evidence of a possible interaction or merger event.  There appears to be a primary, larger component exhibiting an elliptical shape. A secondary, smaller component is visually distinct and slightly offset from the primary galaxy. This secondary component presents a more amorphous, less well-defined structure. Color variations are observed within the system. The primary component exhibits a yellowish-red hue, possibly indicative of an older stellar population or dust obscuration. The secondary component appears bluer, which could indicate regions of more recent star formation. Overall, the galaxy appears to be in an intermediate state of evolution, potentially resulting from ongoing or recent galaxy merging activity.
