The galaxy presents as a relatively smooth, elliptical shape, with a high degree of central concentration. The core appears bright and somewhat diffuse, fading towards the edges. The primary light distribution suggests a spheroid-dominated morphology. Hints of blue tinting are seen in the outer regions, which may indicate some low-level star formation activity. Overall, the galaxy appears to be of moderate size and mass, exhibiting characteristics of a disk galaxy with a low star formation rate. No signs of major mergers or significant tidal disturbances are visible, although a minor irregularity cannot be ruled out. The object is generally elongated, and it is relatively undisturbed. 
