The galaxy presents as a largely smooth, elliptical-like structure, with a high degree of central concentration. Its color profile exhibits a general trend towards redder hues. There is little evidence of distinct spiral arms or strong dust lanes, indicating a relative lack of ongoing star formation. A slight blue tint is visible in regions of the galaxy, potentially indicating pockets of young stars, though the overall contribution to the galaxy's light appears minimal. No strong signs of tidal disturbances or interactions with other galaxies are apparent in the immediate vicinity.
