The galaxy appears as a slightly elongated, elliptical structure. The central region exhibits a high degree of luminosity, indicating a concentrated population of stars. The light distribution appears smooth and relatively uniform, with no obvious spiral arm structure or distinct features. The outer regions of the galaxy gradually fade into the background, suggesting a decrease in stellar density with increasing radius. The color of the galaxy is predominantly yellow, suggestive of an older stellar population. There is a minimal presence of blue, signaling a low rate of ongoing star formation. The galaxy exhibits a notable smoothness with hints of a slight disturbance, but no major merging events or significant morphological irregularities are observed.
