The galaxy presents as a relatively smooth, elliptical object. The color gradient suggests a dominant population of older stars, with a noticeable concentration of light toward the center of the galaxy, indicating a high degree of central mass concentration. The shape is moderately elongated, deviating slightly from a perfectly circular profile. There is no apparent dust lane or spiral arm structure visible. The overall appearance indicates that it is a large, evolved galaxy with a relatively low star formation rate. There is a possible minor disturbance present, but this may be due to an unrelated object.
