The galaxy presents with a generally smooth morphology, though there are some indications of features or substructures that may be merging or indicative of minor disturbances. The overall form appears to be somewhat elliptical. The central region exhibits a concentrated luminosity with a yellow-orange hue, suggesting an older stellar population. Fainter, diffuse extensions appear to stretch outwards, exhibiting some bluish-white regions indicating younger stars with ongoing star formation. Some of the outer regions suggest minor tidal interactions or potential merging events, given the somewhat irregular light distribution. The core shows signs of being relatively massive.
