The galaxy presents as an elliptical morphology. It exhibits a smooth, concentrated light distribution, peaking centrally in a yellow-white hue, indicative of an older stellar population. The radial color gradient suggests bluer regions in the outskirts. No distinct spiral arms or a bar structure are discernible within the observed image resolution, though a slight disk is possible. The galaxy does not obviously appear to be undergoing any major mergers. There is little evidence of active star formation present. The object has a relatively compact size.
