This galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a generally round morphology, lacking any obvious spiral arm structures or significant distortions. The light distribution suggests a primarily older stellar population, with a yellow-red hue indicative of evolved stars. There is no strong evidence of ongoing, large-scale star formation activity; the galaxy appears to be largely quiescent. Subtle color variations might be present, possibly indicating minor differences in stellar populations or dust content within the galaxy, although these are not pronounced. No signs of any major interactions or mergers with other galaxies were apparent.
