The galaxy presents a centrally concentrated structure, likely an elliptical or lenticular morphology. A bright, yellowish core is observed, suggesting an older stellar population with minimal ongoing star formation in the nuclear region. Fainter bluish hues extend outward from the core, hinting at the presence of a disk with some younger stars and regions of active star formation, however this is uncertain given the image quality. No clear spiral arm structures or bar features are discernible. There may be some evidence of minor tidal disturbances. The overall light distribution appears relatively smooth, but some minor irregularities are present.
