The galaxy presents a generally smooth and rounded morphology. The color profile indicates a mature stellar population, trending towards redder hues. There is no clearly defined spiral structure or prominent dust lanes visible, suggesting an elliptical or lenticular classification. There may be some subtle internal variations in color and luminosity, but these are not distinct enough to indicate ongoing major star formation. The overall structure appears relatively undisturbed, with no strong evidence of recent or ongoing merger activity. The galaxy's size is moderate, appearing as a compact object in the field.
