The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. Its shape is oblong, with an axis ratio suggesting a moderate degree of flattening. A bright, concentrated central bulge dominates the galaxy's luminosity profile. Moving outward from the core, the light gradually decreases in intensity. There is a hint of a disk structure. The color gradient indicates an older stellar population, typical of elliptical galaxies. No obvious signs of recent merger activity or significant star formation are observed. The galaxy displays a reddish hue, suggesting a dominance of older, redder stars and minimal dust content.
