The galaxy presents a generally smooth morphology, with a high degree of central concentration. It exhibits an elliptical appearance, deviating from a perfectly circular shape, appearing somewhat elongated. Its color profile indicates a yellow-white core, possibly indicative of an older stellar population. Faint bluish tinges are observed in the outer regions, hinting at the presence of younger, hotter stars. No obvious spiral arms or distinct features, such as dust lanes, are visible. There is no obvious evidence of active merging or major tidal disturbances within the image. The galaxy displays a radial color gradient, becoming bluer towards its outskirts, suggesting ongoing star formation activity beyond the core.
