This galaxy presents as a lenticular or possibly an early-type spiral system, observed at a moderate inclination. The central bulge is prominent and exhibits a relatively smooth, concentrated distribution of light, suggesting an older stellar population. The disk component, while discernible, lacks high-contrast spiral arm features. Instead, it shows a smoother, more diffuse distribution of light. The overall color profile indicates a general lack of significant ongoing star formation, with a redder hue dominating the visual appearance. No strong signs of recent or ongoing major merger activity are evident, although subtle distortions in the disk could indicate past interactions. The galaxy displays a regular, elliptical morphology, with a smooth brightness gradient from the core outward.
