The galaxy presents as a primarily smooth object, with a notable absence of distinct spiral arms or prominent disk-like structures. It exhibits a concentrated central bulge which dominates the light profile. The overall shape appears largely circular or elliptical, deviating only slightly from a perfect sphere. There are no obvious indications of ongoing major mergers or significant tidal disturbances in the immediate vicinity of the galaxy. There is a possibility of minor interactions with a close companion, although it is difficult to discern from this image alone. The galaxy appears to be a relatively isolated system.
