The galaxy presents as a moderately luminous, elongated, and seemingly undisturbed system. Its overall morphology appears smooth and featureless, suggesting a spheroid or elliptical type. There is a prominent central bulge, possibly indicative of a supermassive black hole. The colour profile suggests a galaxy dominated by older stellar populations, trending towards redder hues and relatively low ongoing star formation, with a hint of blue possible at the edges. The galaxy exhibits a high degree of rotational symmetry around its central axis. There is no evidence of recent major mergers or tidal disturbances and the edges seem relatively smooth.