The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. There is minimal visible substructure such as spiral arms or prominent dust lanes. The overall color appears yellowish-red, suggestive of an older stellar population with a lower rate of ongoing star formation. The isophotes, while somewhat irregular, indicate a predominantly spheroidal morphology. There might be a very subtle indication of a faint disk, but its presence is uncertain given the image quality. No strong tidal features are visible, suggesting the absence of recent major mergers. The galaxy appears isolated, without any nearby companions significantly disrupting its morphology.
