The galaxy presents as a relatively compact, early-type system, exhibiting a smooth, featureless morphology. Its overall shape is approximately round, with a slight suggestion of ellipticity. The galaxy's light profile is centrally concentrated, lacking prominent spiral arms or bar structures. There is no evidence of a significant disk component or ongoing major merger activity. A slight disturbance might be present. Color suggests that the galaxy is composed primarily of an older stellar population, with diminished recent star formation activity.
