The galaxy presents as a somewhat diffuse, elliptical structure. A bright, concentrated central bulge is apparent, exhibiting a yellowish hue suggesting an older stellar population. Moving outward from the core, the galaxy transitions into a less defined, fainter halo with a subtle bluish tint, hinting at the presence of younger, hotter stars and possible ongoing star formation, although it appears relatively quiescent. The overall form is more elongated than circular but not particularly stretched, with no prominent spiral arm structures or obvious signs of a recent major merger event visible in the image. There is a faint hint of possible minor disturbance in its shape, indicating a subtle interaction or tidal effect.
