The galaxy appears as a largely spheroidal object. The color profile suggests a dominant population of older stars, with a pronounced central bulge that is bright and slightly redder in color, indicative of a concentration of evolved stars and potentially a supermassive black hole. The outer regions of the galaxy display a fainter, more bluish hue, hinting at a small component of younger, hotter stars. There is little evidence of strong spiral arm structure or significant dust lanes, and the overall texture is smooth, suggesting a relatively relaxed morphology. The object shows no strong signs of tidal disturbances or ongoing mergers with other galaxies. The galaxy's shape is generally round. Overall, this appears to be an elliptical or lenticular galaxy at an intermediate redshift.