The galaxy presents as a relatively smooth, elliptical structure with a high degree of roundness. There is no apparent spiral arm structure or significant disk component visible in the imagery. The color profile suggests an older stellar population, as indicated by the reddish-yellow hue. A small area of blue indicates an area of some younger stars. The galaxy appears to be fairly isolated, showing no significant signs of tidal disturbances or interactions with other galaxies, although a couple of possible tidal arms are present. Overall, the galaxy exhibits a morphology consistent with an evolved system, likely with a relatively low ongoing star formation rate.
