The galaxy presents as an elliptical morphology, appearing largely smooth in structure. The color profile indicates a higher concentration of older stellar populations, exhibiting a yellow-red hue. The overall form is more elongated than spherical, but not distinctly cigar-shaped. No prominent spiral arms, dust lanes, or active star-forming regions are discernible within the galaxy's structure. There is no indication of tidal tails or other signs of recent major mergers. There may be some minor asymmetry in the outer halo. The galaxy's compact size and smooth texture could indicate a relatively passive state with low star formation.
