The galaxy presents as a relatively smooth, elliptical form. Its light distribution suggests a centrally concentrated bulge, gradually fading towards the outer edges. The galaxy appears to be generally rounded in shape. There are no obvious spiral arms or disk-like structures visually apparent. There may be some minor disturbances within the structure of this galaxy, but no major disturbances or signs of an active merger are immediately evident. The overall color suggests a population of older stars, potentially indicating a lower current star formation rate.
