The galaxy presents as a relatively compact object with an apparent smooth morphology. Its shape appears to be that of a flattened spheroid, likely an elliptical galaxy or a lenticular galaxy viewed at an oblique angle. There appears to be a central concentration of light, suggesting a bulge component. There may be a faint disk component, however it cannot be determined due to the image quality. The color gradient suggests that the central region of the galaxy exhibits a slightly more yellow hue compared to the outer regions, potentially indicating an older stellar population centrally. There is no obvious evidence of spiral arm structure or ongoing star formation. No significant tidal disturbances or evidence of interaction with other galaxies is visible.
