The galaxy presents a generally smooth morphology, exhibiting a high degree of central concentration. The light distribution appears largely elliptical, with a fairly symmetrical structure radiating outward from a bright, compact core. The core region displays a yellowish-orange hue, potentially indicative of an older stellar population. Fainter, diffuse emission extends outwards from the core, showing a slight color gradient towards redder tones in the outer regions, possibly signifying a change in stellar population or dust content with increasing radial distance. There is little evidence of prominent spiral arms or significant dust lanes; however, subtle irregularities in the outer isophotes might suggest minor tidal disturbances or past interactions. Based on the observed morphology, it is likely an elliptical galaxy, possessing substantial mass and a relatively low star formation rate.
