The galaxy presents a relatively smooth, elliptical morphology with a slight elongation. Its color profile suggests a predominantly older stellar population, exhibiting a yellowish-red hue, potentially indicating a lack of significant recent star formation. There is little evidence of spiral arms or a prominent disk structure. A concentration of light toward the central region suggests a bulge. No signs of major mergers or tidal disturbances are apparent, suggesting a stable, relatively undisturbed system.
