The galaxy presents as a relatively smooth, elliptical structure with a bright, concentrated central bulge. There is a subtle flattening observed, with the major axis extending roughly horizontally across the image.  The luminosity appears to decrease steadily from the core outwards. The core region exhibits a yellowish hue, possibly indicating an older stellar population and lower star formation rate.  Moving outwards, there is an indication of a slight disk-like structure with spiral arms. These arms are not well-defined and lack the clumpy structures typically associated with active star-forming regions. Overall, the galaxy appears to be relatively quiescent. There is no evidence of active galactic nuclei activity, strong tidal features, or recent major merger events. The galaxy presents a moderate level of disturbance in its morphology.