The galaxy presents as a yellowish, relatively smooth object with a centrally concentrated luminosity profile. The light distribution suggests an elliptical morphology, appearing mostly regular with minimal visible substructure. A slight elongation is discernible, indicating it's not perfectly spherical, tending more toward an intermediate sphericity. There is no apparent spiral arm structure or significant dust lane obscuration. The overall appearance suggests a system dominated by an older stellar population with ongoing, but relatively low, levels of star formation. No obvious signs of a recent major merger or significant tidal disturbance are apparent. Faint extensions or a very subtle halo might be present, but it is difficult to be certain due to the image resolution.
