The galaxy presents as a relatively smooth object with a high degree of central concentration. It exhibits an overall elliptical morphology, with a slight elongation. The core region appears bright and yellowish, potentially indicating a population of older stars. The outer regions are less luminous and exhibit a blueish tint which may indicate some recent star formation. There are no distinct spiral arms or bar structures visible. The galaxy appears to be relatively isolated, with no obvious signs of interaction or tidal disturbances.
