The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its shape is approximately round, with a slight deviation towards a mild ellipticity. A dominant central bulge is evident, exhibiting a yellowish hue, suggesting a population of older stars. Fainter, bluish light extends outwards from the core, which could indicate some ongoing, albeit low, levels of star formation in the outer regions. There is no discernible spiral structure or prominent dust lanes visible in the image. No significant tidal features or indications of recent major merger activity are apparent. A subtle asymmetry is noted, hinting at a minor gravitational interaction or internal disturbance. The overall color profile suggests an intermediate population of stars with both young and old components.
