The galaxy presents a smooth, largely featureless morphology. It exhibits a roughly elliptical shape with a high degree of roundness. A distinct central bulge region is observed, appearing significantly brighter and more concentrated than the surrounding halo. The color profile suggests a population of older stars, indicated by the yellowish-red hue, particularly concentrated in the galactic center. Faint bluish tinges in the outer regions may suggest areas of limited, ongoing star formation, though this activity appears subdued overall. There is no visible evidence of significant tidal disturbances, major mergers, or prominent spiral arm structures. The galaxy appears relatively isolated and undisturbed.
