The galaxy presents as a somewhat irregular object, appearing to be in a state of interaction or merger. The central region displays a brighter, more concentrated luminosity. Evident are multiple distinct luminous cores or knots. There are indications of disturbed morphology; it may have features that suggests tidal tails or disrupted spiral arms which cannot be distinguished with certainty due to the image's resolution. The overall color profile tends towards the redder end of the spectrum, with distinct yellower components. This coloration suggests an older stellar population. The galaxy is not a perfectly smooth, elliptical object. Some degree of ongoing star formation is not incompatible with the color and morphology observed, although it likely hosts an aging stellar population on average. There is a prominent and distinct companion object.
