The galaxy presents as a generally smooth, elliptical-like structure with an approximate half-light radius estimated around 13 kpc. The overall color is yellowish-orange suggesting an older stellar population, indicative of diminished recent star formation. There is a very subtle central concentration of light. No distinct spiral arms or bar structures are apparent. Faint extensions around the primary body can be seen but they appear quite amorphous, possibly due to minor gravitational interactions. The galaxy doesn't appear to be undergoing any significant merger events based on the relative lack of strong tidal features. There is little evidence of ongoing or recent high levels of star formation.
