The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The light distribution is dominated by a yellowish-orange hue, indicative of an older stellar population. There are no obvious spiral arms or dust lanes visible. The isophotes appear relatively regular and symmetric, suggesting a relaxed morphology without significant ongoing mergers or tidal disturbances. The galaxy exhibits a high degree of roundness in its overall shape. Faint bluish light is visible towards the outer regions, hinting at some younger, hotter stars and ongoing star formation.
