The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology with a high degree of central concentration. The core region displays a bright, yellowish hue, suggesting an older stellar population. The outer regions show a gradual decrease in surface brightness, transitioning to a slightly bluer color, indicative of a possible younger stellar component within the disk. The shape is closer to an in between roundness, with a slight elongation suggesting it is not perfectly spherical. There is no obvious evidence of ongoing major mergers or strong tidal disturbances. Faint hints of a disk-like structure are possibly present, making it difficult to classify precisely.
