The galaxy presents a roughly elliptical morphology, viewed at a near edge-on inclination. The central region exhibits a high surface brightness, appearing nearly uniform and featureless in the available data. Diffuse light extends outward from this core, forming a somewhat flattened disk-like structure. 

Faint, extended emission is observed beyond the main body of the galaxy, but it appears disturbed and asymmetrical on one side. This may be an indication of tidal interactions or recent minor merger activity. However, the galaxy's internal structure does not show distinct spiral arms or bar features. The galaxy displays a color gradient, with the central bulge appearing redder than the outer disk. The overall color suggests a mix of stellar populations, with an older, more evolved population concentrated in the center and younger stars in the disk. 
