The galaxy presents a largely smooth, elliptical morphology. It appears highly concentrated, with a bright, yellowish core that gradually fades into the surrounding galactic halo. There is little to no evidence of distinct spiral arm structures or prominent dust lanes. The overall shape is predominantly round, exhibiting minimal elongation or asymmetry. The galaxy’s color profile indicates a population of older stars, primarily redder in color. No signs of active star formation are easily discernable. There are no evident signs of tidal disturbances or interactions with neighboring galaxies, suggesting a period of relative isolation and quiescence. There may be a weak, faint ring feature at the outer edge of the galaxy, but this is difficult to distinguish.
