The galaxy presents as a generally smooth, elliptical form. The light distribution suggests a concentration of stars toward the center, forming a bright, prominent nucleus. The galaxy appears to be slightly elongated, deviating from a perfectly circular shape. The color gradient shifts from a yellowish-white core to a slightly redder hue in the outer regions. There is no clear evidence of spiral arms or prominent dust lanes. Faint disturbances are not obvious, but it's unclear if they are present within its structure.
