The galaxy presents an overall elliptical morphology, appearing largely smooth and homogenous in structure. The core exhibits a high degree of central concentration, with a bright, yellowish-orange hue suggesting an older stellar population. The outer regions transition to a fainter, more diffuse halo. There is a slight elongation to the galaxy's shape; it is not perfectly spherical, tending towards a cigar shape. No distinct spiral arm structures or prominent dust lanes are discernible within the available image resolution. There is minimal evidence of any major ongoing merger activity or significant tidal disturbance, although some minor irregularities in the outer halo cannot be entirely ruled out. There is evidence of star formation.
