The galaxy presents a predominantly smooth morphology, with a suggestion of elliptical shape. It exhibits a high degree of central concentration of light, fading gradually towards the outer edges. The color profile suggests an older stellar population, with a yellowish hue dominating the central region, consistent with a lack of significant ongoing star formation. Faint hints of a disk-like structure might be present but not clearly defined. No apparent tidal features or signs of major mergers are visible; though a minor disturbance can't be ruled out. Overall, the galaxy appears to be relatively isolated.
