The galaxy presents as a moderately bright, elliptical form with a smooth overall appearance. The light distribution suggests a fairly even stellar population density, concentrated centrally, fading towards the outer edges. The galaxy appears to be generally spheroid, with an intermediate roundness. There is a suggestion of some internal structure, although not clearly defined. No strong evidence of spiral arms or a distinct disk component is observed. The color profile indicates a mix of stellar populations, with a central, slightly redder hue potentially indicating older stars. The outer regions show bluer hues, suggesting a younger population. There appear to be no significant interactions or merger events evident in this observation, with the galaxy appearing relatively isolated and undisturbed.
