The galaxy presents a generally smooth and concentrated morphology. The light distribution is dominated by a central, bright, yellowish core, indicative of an older stellar population. Extending outwards from this core, a diffuse and less luminous envelope is visible, appearing somewhat elongated in shape. Subtle variations in color suggest possible differences in stellar population or dust content within this outer region, with a slightly redder hue apparent. There is no clear evidence of distinct spiral arms or a prominent disk structure. The overall impression is that of an elliptical or lenticular galaxy, displaying a relatively quiescent state with low star formation activity. Minor distortions in the outer regions cannot be ruled out.
