The galaxy presents a primarily smooth, elliptical morphology, appearing as a spheroid of light with a concentrated central bulge. The color profile indicates a general red-shifted spectral distribution, with a yellowish-orange hue dominating the central region, and a gradient towards redder tones in the surrounding halo. There appears to be some minor visual disturbance and it may be undergoing or have undergone a minor merger. No strong evidence of active star formation regions or distinct spiral arm structures are apparent within the confines of the galaxy.
