The galaxy presents a largely smooth morphology, with minimal discernible substructure. The central region exhibits a concentrated luminosity profile, appearing quite bright with a yellowish hue. Moving outwards from the core, the galaxy's luminosity gradually diminishes into a more diffuse halo. The overall shape appears generally elliptical, exhibiting a moderate degree of roundness. There is no obvious indication of any major merger events or significant tidal disturbances affecting the galaxy’s morphology. Based on color gradients, this galaxy could be a lenticular or elliptical type with moderate mass and low star formation activity.
