The galaxy presents as a moderately bright, elliptical-like structure with a smooth, diffuse morphology. A concentrated, bright central bulge dominates the overall luminosity.  Moving outward from the core, the intensity of light gradually diminishes, fading into a fainter, more extended halo. The galaxy appears elongated, with a relatively high degree of apparent roundness. There is no discernible evidence of spiral arms, bars, or distinct features indicative of active star formation regions like HII regions or dust lanes, but there is a smooth blue halo around the core of the galaxy. There are no visible signs of any major mergers. The galaxy has a general smooth appearance. 
