The galaxy presents as a somewhat elongated, ellipsoidal structure with a central concentration of light. The core region exhibits a yellowish-white hue, suggesting an older stellar population. Progressing outward from the core, the color shifts towards a bluer, less saturated tone. This implies a population of younger, bluer stars in the outer regions, although the transition appears relatively smooth and not indicative of prominent spiral arm structures. The overall morphology suggests a lenticular or early-type spiral galaxy, possibly seen at a slight angle. There is no visually discernible evidence of strong tidal interactions or ongoing major mergers. The overall light distribution is relatively smooth, with only subtle variations in brightness across the galactic disk.
