The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated, bright central bulge that dominates the overall luminosity. The light profile suggests a relatively even distribution, with a gradual decrease in intensity moving outward from the core. The galaxy shows some features which could be described as minor disturbances. In terms of color, the galaxy appears to be dominated by redder wavelengths, indicating a population of older stars and a suppressed rate of star formation. The isophotes are generally round to slightly elliptical in shape. The image reveals no prominent spiral arm structures or significant dust lane obscuration.
