The galaxy exhibits a distinct elongated, cigar-like morphology, suggesting it is likely an elliptical galaxy, viewed at an angle. The primary color appears to be a yellowish-white, with the core of the galaxy appearing a more concentrated yellow. This color suggests an older stellar population, with minimal ongoing star formation. There is a high degree of smoothness in the galaxy's light distribution, with no prominent spiral arms or distinct features visible. There is no visual evidence of a major ongoing merger. Slight disturbances may be present, but not definitively.
