The galaxy presents a generally smooth, elliptical morphology. Its light profile suggests a centrally concentrated structure, with a gradual decrease in surface brightness moving outward from the core. The color gradient indicates a redder core, potentially indicative of an older stellar population or increased dust obscuration. Moving outward from the core, the galaxy exhibits bluer colors, suggesting the presence of younger stars. The galaxy displays a slight elongation, classifying it as an elliptical galaxy of type E4 or E5 on the Hubble sequence. There is no obvious evidence of significant star formation activity or tidal disturbances indicative of a recent merger event; the galaxy appears to be a relatively undisturbed system.
