The galaxy presents as a concentrated, elliptical morphology. It exhibits a smooth, relatively featureless light distribution, lacking prominent spiral arms or a distinct central bulge. The color profile suggests a dominant population of older stars, indicated by the yellowish hue. There is little evidence of significant ongoing star formation activity. The galaxy displays a moderate degree of roundness, tending towards an elliptical shape rather than a highly flattened disk or elongated form. No major disturbances or signs of recent merging events are readily apparent in its structure.
