The galaxy presents as a relatively smooth and centrally concentrated structure, with a notable absence of distinct spiral arms or a prominent disk. The light distribution appears centrally dominant with an elliptical morphology. The galaxy's color profile suggests a population of older stars, indicated by a redder hue. Overall, the galaxy appears to be a relatively mature system, likely an elliptical galaxy or a lenticular galaxy viewed at a high inclination, showing little evidence of recent star formation.
