The galaxy presents as a singular, relatively symmetrical entity. Its morphology appears largely smooth and elliptical, with a high degree of central concentration. The core exhibits a bright, yellowish hue, indicative of an older stellar population. Radially outward from the core, the color transitions toward a slightly redder tone. There is no discernible disk structure, spiral arms, or prominent dust lanes. Some asymmetry can be seen in the outer edges, but it does not seem to have any major disturbances. The overall impression is that of a well-defined, evolved system.
