The galaxy presents a largely smooth morphology, with no apparent spiral arms or significant disk structures visible at this resolution. It appears elliptical or spheroidal in shape, exhibiting a high degree of roundness. There is a color gradient observed, with a central region exhibiting a yellowish or golden hue, suggesting an older stellar population. The outer regions appear dimmer and slightly redder, indicating a less intense and perhaps more dispersed distribution of stars. There is no noticeable dust lane, bar or indication of any merger events. The lack of observable disk features and prevalence of a smooth, rounded structure points towards classification as an elliptical galaxy, characterized by a dominant spheroidal component and minimal ongoing star formation.
