The galaxy appears as a single, concentrated luminous body with a largely featureless morphology. It exhibits a centrally concentrated brightness profile, suggestive of a significant bulge component. The galaxy's overall shape is approximately round. There is a color gradient from a yellow/white core to bluish hues in the outer regions, possibly indicating younger stellar populations are present outside of the central regions. There is no apparent spiral arm structure or bar. There are no signs of tidal tails, or other major disturbances. The galaxy likely has a moderate mass and a modest amount of on-going star formation activity.
