This galaxy presents as a largely homogenous elliptical system, exhibiting a smooth, concentrated morphology. Its overall shape is notably round. A distinct central bulge is visible, characterized by a bright, concentrated luminosity that gradually decreases toward the outer regions. The galaxy shows no apparent spiral arm structures, nor does it display any obvious signs of ongoing merging events or major disturbances. The color profile indicates a higher concentration of older stellar populations, contributing to a redder overall hue. There are no visible dust lanes or prominent star-forming regions within the galaxy's disk.
