The galaxy presents as a centrally concentrated, luminous object with a generally smooth appearance. It exhibits a roughly elliptical morphology, appearing nearly circular. The core displays a bright, yellowish-white hue, suggesting an older stellar population. The outer regions transition to a dimmer, reddish color, indicating the potential presence of a cooler stellar population or dust attenuation. There is no clear evidence of spiral arms or prominent disk structures. Faint, diffuse extensions of light are visible in the surrounding halo, though without significant irregularities or signs of ongoing merger activity. The general morphology suggests this galaxy is likely an elliptical galaxy, potentially exhibiting a relatively low rate of star formation.
