This galaxy appears as a moderately bright, relatively smooth elliptical galaxy, with an estimated effective radius of approximately 4.4 kpc. It exhibits a spheroidal morphology with a high degree of roundness. There is no discernible disk structure, nor any prominent spiral arms. 

There is a subtle, diffused halo surrounding the central region of the galaxy. No signs of ongoing major merger events are immediately obvious, though a minor interaction or tidal disturbance cannot be ruled out due to slight irregular morphology. The galaxy presents a color profile consistent with a population of older stars, with little evidence of significant recent star formation. The overall color is moderately red.
