The galaxy presents as a largely smooth object, characterized by a centrally concentrated bulge. The overall shape approximates a circular form, exhibiting high degree of sphericity. No distinct spiral arm structure or prominent disk features are readily apparent within the optical data. There is a subtle suggestion of disturbance in the outer halo region, though it is difficult to characterize. The galaxy exhibits a redder color, suggesting an older stellar population and a relatively low ongoing star formation rate. The galaxy appears to be a massive system, given its significant luminosity and extended size.
