The galaxy appears as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge and lacks distinct spiral arm features. The galaxy's color profile suggests a population of older stars, with a redder hue dominant throughout the galactic body. There's a subtle elongation present, indicating it is not perfectly spherical, trending more towards an intermediate elliptical shape. No significant signs of active galactic nuclei or recent major mergers are visually apparent, though subtle disturbances may be present within the outer regions of the galaxy. The size appears moderately large, indicative of a massive galaxy. Star formation appears relatively subdued, given the smooth morphology and color profile. 
