The galaxy presents a generally smooth, elliptical morphology with a notable lack of prominent spiral arms or a well-defined disk structure. The light distribution appears centrally concentrated, fading gradually towards the outer regions of the galaxy. The central region exhibits a brighter, somewhat bluer hue, suggesting the presence of a younger stellar population and potentially ongoing, low-level star formation activity. There's no indication of strong dust lanes or tidal features, supporting the classification as a relatively undisturbed galaxy. Based on the overall color profile and morphology, this galaxy is likely a massive galaxy with a substantial stellar mass, experiencing low levels of star formation.
