The galaxy presents a generally smooth and rounded morphology, indicative of an elliptical or lenticular classification. There are some indications of possible minor disturbances within the structure, but these are not prominent enough to classify it as a major merger event. The color profile appears to be trending towards redder wavelengths, implying a population of older stars and relatively low levels of current star formation. The size, while limited by image resolution, appears to be consistent with a galaxy of moderate size. Overall, the galaxy appears to be a relatively evolved system, approaching a more quiescent state.
