The galaxy presents a generally smooth, elliptical morphology. Its light is concentrated toward the center, suggesting a prominent bulge. The galaxy exhibits a somewhat circular appearance, deviating only slightly from a perfect circle. The color profile indicates a population of older stars. The faintness indicates the presence of some star formation, though likely at a low rate. There is no evidence of any major ongoing mergers or tidal disturbances. The galaxy displays a fairly even light distribution throughout its visible extent, implying a well-mixed stellar population.
