The galaxy appears as a centrally concentrated object, exhibiting a generally elliptical morphology. Its light profile transitions smoothly from a bright, relatively yellow core outwards. Fainter, diffuse bluish hues can be detected surrounding this core. The overall structure lacks any obvious spiral arms or prominent disk-like features. There is no sign of tidal disturbances or interaction with any nearby neighbors. The galaxy appears relatively isolated and relaxed. The color suggests an older stellar population is dominant but with the presence of some young star formation.
