The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. Its color profile suggests a dominant population of older stars, with a yellowish hue concentrated toward the core. A slight elongation is perceptible, deviating from a perfectly circular shape, although the galaxy appears primarily elliptical. There is no obvious indication of active star formation regions nor prominent spiral arm structures within the visible light spectrum. The galaxy lacks any signs of a recent or ongoing major merger event, indicating relative gravitational stability. The galaxy's structure is dominated by a smooth stellar distribution.
