The galaxy presents a generally smooth, elliptical morphology. Its light profile exhibits a centrally concentrated brightness that decreases gradually with radial distance. There is no apparent spiral structure or distinct disk component visible at this resolution. The color is predominantly yellow, which might suggest an older stellar population with reduced ongoing star formation. There is a slight deviation from perfect circularity, tending toward a slightly elongated, though not cigar-shaped, profile. There is no strong evidence of tidal features, major disturbances, or ongoing merger activity based on this image. The smooth appearance suggests the galaxy is relatively relaxed, dynamically.
