The galaxy presents as an elongated, elliptical structure. It appears generally smooth in texture, lacking significant granular features or spiral arm structures within its visible extent. The central region exhibits a concentration of light, suggesting a prominent galactic bulge. The color profile leans toward warmer hues, with a yellowish-orange core potentially indicative of an older stellar population. Fainter, blue-ish regions surround the core, suggestive of more recent star formation. The galaxy appears relatively isolated, showing no immediately obvious signs of major tidal interactions or mergers, although subtle disturbances may be present upon closer inspection. Its elongated shape implies a degree of intrinsic asymmetry or an inclined viewing angle with respect to our line of sight.
