The galaxy presents as a smooth, elliptical structure with a concentrated central bulge. The light distribution is relatively uniform, lacking prominent spiral arms or distinct features. There's an apparent radial color gradient; the core appears yellowish-orange, suggestive of an older stellar population. Moving outward, the color gradually transitions to a slightly redder hue. The galaxy exhibits a high degree of roundness and a lack of any major morphological disturbances, with an estimated diameter of approximately 6.6 kpc. Overall, the light profile suggests a galaxy with a fairly suppressed rate of star formation.
