This galaxy presents a somewhat amorphous, though roughly elliptical morphology. The light distribution appears to be dominated by a smooth, centrally concentrated bulge. There is a hint of a disk-like structure, but it appears significantly disturbed or disrupted. The color profile indicates a population of older stars, visible by the reddish hue in the central region of the galaxy. There are suggestions of recent merger activity, with a slightly asymmetrical shape. The galaxy exhibits some faint features that might be tidal tails or debris associated with an interaction or merger event. There is no strong evidence of active star formation in the galaxy's visible structure.
