The galaxy presents as a slightly elongated, likely elliptical, morphology. The core exhibits a concentrated, yellowish-orange hue, suggesting an older stellar population and minimal ongoing star formation within the central region. The isophotes appear relatively smooth and regular, with a gradual decrease in surface brightness outward from the core. There is faint evidence of a very subtle disk-like structure extending along the major axis, although this is not the dominant feature. The galaxy's overall color profile indicates a relatively evolved system with moderate mass, and low star formation rate. There is no obvious indication of any significant merger activity or tidal disturbances.
