The observed galaxy presents a largely smooth and featureless morphology. The color profile suggests a population of older stars, exhibiting a reddish-yellow hue concentrated towards the galactic center. The overall shape is elliptical, appearing somewhat elongated rather than perfectly spherical. There's no clear evidence of a prominent disk structure or spiral arms. Faint irregular blueish color variations at its periphery suggests the presence of sparse, ongoing star formation activity, though relatively low. The galaxy appears isolated, showing no strong indications of recent or ongoing major mergers with other galaxies. There is a possible minor tidal disturbance or weak gravitational interaction but it appears negligible.
