The galaxy presents a generally smooth morphology, appearing elliptical in shape with an approximate semi-major axis of 6 kpc. The light distribution is centrally concentrated, with a peak in the yellow-orange wavelengths at the core, suggesting a dominant population of older stars. There is very little evidence of spiral arm structure or significant dust lanes within the galaxy. The overall color gradient from the core to the outer regions is subtle, showing a slight decrease in the redder wavelengths and a relative increase in bluer wavelengths. There is no clear sign of active galactic nuclei or other major disturbances of this galaxy.
