The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology with a noticeable absence of distinct spiral arms or a prominent disk structure. The light is more concentrated at the center. The color profile suggests a population of older stars and a relatively low rate of ongoing star formation, as evidenced by the redder hue of the galaxy. The apparent size is small, but this is affected by redshift and distance. There is little evidence of any major disturbances or merging events in its recent past, based on the smoothness of the galaxy's overall form.
