This galaxy appears to be a relatively luminous, isolated system. Its morphology is smooth and elliptical in nature. The light is concentrated towards the center in a bright core, decreasing gradually outward. The galaxy has a yellow hue to it, which fades slightly as it reaches the outer edges. The smooth profile suggests the galaxy has an older stellar population, consistent with a lack of significant ongoing star formation. There is no evidence of spiral arms or a prominent dust lane. The galaxy appears largely undisturbed, showing no major signs of tidal interactions or recent mergers. The overall shape is somewhat elongated but relatively close to round, with no obvious distortions.
