The galaxy presents as an elliptical morphology, with a smooth and concentrated central bulge that emits primarily yellow-white light. This suggests an older stellar population within the bulge. The overall shape appears somewhat elongated, tending toward a cigar shape rather than perfectly round. A faint, diffuse disk surrounds the central bulge, exhibiting a bluer hue. This hints at the presence of some ongoing star formation activity, although at a low rate, with younger, bluer stars residing in the disk. No distinct spiral arm structures are observed. There are no obvious signs of any major merger events or significant tidal disturbances, though a minor interaction cannot be completely ruled out. 
