The galaxy presents a generally smooth and rounded appearance. It appears as a concentrated mass of light with no obvious spiral arm structure or prominent disk features visible. There is a slight deviation from perfect circularity, with a hint of elongation or an intermediate form. Color gradients suggest varying stellar populations across the galaxy's body, although the overall color profile is somewhat homogenous. A hint of blue light indicates some regions of ongoing star formation, although the galaxy appears mostly redder in color, implying that it is largely composed of older stars. There appears to be little tidal disturbance or evidence of a major ongoing merger with another galaxy. The galaxy shows some indication of minor disturbances to its morphology.
