The galaxy presents as a single, largely featureless entity. The color profile suggests a primarily older stellar population, with the bulk of the light emanating from the yellow-red portion of the spectrum, indicative of evolved stars. There is some evidence of bluer light in the central region, which may indicate some recent, however limited, star formation. The overall shape is close to circular, lacking any clear spiral arm structure or a pronounced disk. There are no signs of tidal tails or other significant morphological disturbances, indicating it is a relatively undisturbed system, with no major merging events.
