The galaxy presents as a centrally concentrated structure, appearing generally smooth in morphology. There is a dominant, bright central bulge that is yellowish, likely indicating an older stellar population. The galaxy is moderately elliptical in shape, showing some deviation from a perfectly circular appearance. Faint, diffuse light surrounds the central bulge, suggesting an extended halo or a very faint disk. No distinct spiral arms or significant dust lanes are discernible in the available imagery. The overall color profile suggests a lack of significant ongoing star formation. There may be some minor disturbances in the overall structure, but no major signs of merging are evident.
