The galaxy presents a generally elliptical morphology, appearing relatively smooth and rounded in structure. There is a concentration of luminosity towards the central region, indicative of a prominent galactic bulge. The color profile suggests an older stellar population, trending towards redder hues with minimal evidence of active star formation regions detectable within the available image resolution. There is no apparent disk structure, or significant dust lanes. No tidal features or signs of recent merger activity are readily observable.
