The galaxy presents a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a well-defined disk structure. The color profile suggests a relatively red population, indicative of older stars and a lower rate of ongoing star formation. The overall shape is generally rounded, with a slight tendency toward elongation. There is some evidence of minor disturbance in the galaxy's structure, possibly indicating past interactions or mergers. The galaxy has a central bulge which dominates the galaxy's light.
