The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. There is a slight elongation, though it appears mostly round. The galaxy exhibits a yellowish hue, suggesting an older stellar population and/or the presence of dust obscuration. No obvious spiral arm structures or significant star-forming regions are visible. The overall light distribution is diffuse, lacking distinct features that would indicate recent merger activity or significant tidal disturbances. The galaxy is relatively compact in size.
