The galaxy presents as a slightly elongated structure. Its morphology is not perfectly smooth, showing some indication of features, possibly disk-like or irregular. There is a hint of a central bulge that appears brighter and somewhat concentrated. The galaxy displays a redder hue, suggesting a population of older stars and/or a significant amount of dust obscuring younger, bluer stars. The overall shape leans towards being cigar-shaped rather than perfectly round, indicating it could be an elliptical galaxy or possibly a spiral viewed edge-on with significant disturbance. There is no strong evidence of major merging activity, though some minor disturbance can't be excluded. Based on these properties, it can be inferred that this galaxy may have a significant mass and a moderate rate of star formation.
