The galaxy presents an overall elliptical morphology, appearing largely smooth in texture with a high degree of central concentration. The core exhibits a bright, yellowish-white luminosity, suggestive of an older stellar population. This central region transitions gradually into a fainter, less defined halo. Faint bluish tones are observed at the outermost edges. The galaxy shows no apparent signs of spiral arms or bar structures and no evidence of any significant ongoing merger events or strong tidal disturbances. It has a relatively regular, rounded shape. There may be some minor irregularities on one edge, indicative of a subtle disturbance or minor interaction.
