The galaxy presents a largely smooth, elliptical morphology, although some slight elongation is apparent, trending towards a cigar shape. Its color profile reveals a relatively redder central bulge, suggesting an older stellar population concentrated in that region. Moving outwards, the galaxy appears less red, hinting at the presence of younger, bluer stars in the outer regions. Overall, the galaxy does not show strong indications of any major merger events or significant disturbances, appearing fairly quiescent. However, it does not appear perfectly circular in shape.
