The galaxy presents a primarily smooth morphology, with some subtle features indicative of a disk. The galaxy's shape appears generally round, exhibiting only slight elongation. There is no strong evidence of ongoing major merging activity, though subtle asymmetries might suggest minor disturbances or interactions.

Color gradients indicate a brighter, potentially older stellar population concentrated in the core region, as evidenced by the brighter white light there. There is some presence of bluer light within the disk implying ongoing low-level star formation. The galaxy's relatively high mass and moderate star formation rate suggest it is on the red sequence or in the process of transitioning to it. 
