The galaxy presents a generally smooth and rounded morphology. A central bulge is visible, exhibiting a brighter, more concentrated luminosity. The overall color suggests a population of older stars, shifting towards redder wavelengths. A faint disk component may be present, but the overall structure lacks prominent spiral arms or distinct features. There is no immediate visual evidence of a major ongoing merger event, although some subtle disturbances might be present in the outer regions upon closer inspection. The galaxy appears to be relatively isolated, without any nearby interacting companions immediately apparent in this image.
