The galaxy presents as a diffuse, somewhat amorphous object with a subtly elongated morphology. The central region exhibits a higher surface brightness, appearing nearly spheroidal and gradually fading into a less distinct outer halo. Faint blue-ish hues can be observed in the disk region, suggesting the presence of younger stellar populations or regions of ongoing star formation activity. There is no obvious spiral structure or well-defined bar. The overall appearance leans towards a late-type galaxy that is moderately inclined relative to our line of sight.