The galaxy presents a largely smooth, elliptical morphology. It appears highly rounded in shape with no discernible disk structure or spiral arms. A bright central bulge dominates the overall light profile, suggesting a concentration of older stars. The color is generally consistent with a population of aging stars, exhibiting a yellowish-red hue. There is little evidence of ongoing star formation or dust lanes. The overall structure indicates a gravitationally relaxed system, consistent with an evolved galaxy that has undergone significant merging or secular evolution in the past. No signs of tidal tails or active galactic nuclei are apparent.
