The galaxy presents a largely smooth, elliptical morphology. Its core exhibits a concentrated luminosity, characterized by a distinct reddish-yellow hue, suggesting a population of older stars and a diminished rate of ongoing star formation.  A slight extension is visible to the lower right of the core, displaying a bluish tint. This may indicate a region of more active star formation or a population of younger, hotter stars. Overall, the galaxy appears relatively isolated with no obvious signs of major merger activity, though a slight asymmetry could suggest minor gravitational interaction or internal disturbances. The galaxy possesses a substantial mass.
