The galaxy presents a predominantly smooth morphology. It appears elliptical or lenticular in shape, with a relatively high degree of central concentration. The color gradient suggests an older stellar population, with a slightly redder core transitioning to bluer outer regions. There are no distinct spiral arm structures visible, indicating a lack of ongoing major star formation in a disk component. There is a slight asymmetry within the galaxy's light distribution, possibly indicative of a minor disturbance or past merger event. The galaxy appears relatively isolated, with no obvious signs of a major ongoing interaction with any other large galaxy.
