The galaxy presents a largely smooth, elliptical morphology with a bright, concentrated central region. This core exhibits a slightly reddish hue, potentially indicating an older stellar population. Extending outward from the core, a fainter, bluish halo is observed, suggesting the presence of a younger, bluer stellar population at the periphery. There's evidence of a slight disturbance in the outer regions, possibly indicating a past or ongoing interaction. The overall shape appears somewhat elongated, deviating slightly from a perfect sphere, and tending towards a cigar shape. The galaxy does not appear to have a prominent spiral structure, but is better described as a mostly smooth elliptical galaxy with some disturbances. 
