The galaxy presents as a fairly smooth, elliptical structure. It is characterized by a centrally concentrated bulge that gradually fades into a diffuse halo. The core exhibits a yellowish hue, suggesting an older stellar population. No distinct spiral arms or prominent dust lanes are visible. The overall morphology indicates a relatively evolved system, with little evidence of ongoing major star formation. The galaxy's shape is slightly elongated. Indications of disturbance are minimal. 
