The galaxy presents a generally smooth, elliptical morphology. Its color profile appears relatively uniform, with a slight reddening towards the central region, suggesting an older stellar population. The galaxy exhibits no apparent spiral arm structures, dust lanes, or other features indicative of active star formation. The object is moderately luminous, and likely possesses a significant stellar mass. There is no apparent evidence of any on-going mergers or tidal disturbances, although a subtle asymmetry cannot be ruled out. The object appears to be isolated.
