The galaxy presents a generally smooth morphology, with a high degree of central concentration. The shape appears to be elliptical, exhibiting a deviation from perfect circularity towards a more elongated, cigar-shaped form. There is a bright, concentrated core which suggests a significant density of stars and possibly a supermassive black hole at the galactic center. A subtle color gradient is observed, with a slightly bluer hue towards the outer regions of the galaxy, suggesting a potential presence of younger stellar populations in these areas compared to the core. The galaxy does not appear to be undergoing any major merging events or showing signs of significant tidal disturbances. The outer halo fades gradually into the background, indicating a smooth stellar density profile.
