The galaxy presents as a relatively smooth, centrally concentrated object with a high degree of radial symmetry. Its morphology appears primarily elliptical, tending toward a more spheroidal shape rather than a highly flattened disk. There is minimal evidence of spiral arm structure or significant dust lanes within the galaxy. The central bulge region exhibits a brighter luminosity, gradually fading towards the outer edges. There is a suggestion of minor disturbances, but the dominant form remains that of a relatively relaxed system. The color profile indicates the galaxy is possibly a red sequence galaxy, with the light being generally redder on average.
