The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a largely elliptical morphology, appearing fairly round with only a slight elongation. The light distribution suggests a dominant spheroid component. There is little evidence of distinct spiral arms or a prominent disk structure. The galaxy displays a color gradient, becoming slightly bluer towards its outer regions, possibly indicating some ongoing, albeit low-level, star formation. No significant tidal features or interactions with nearby galaxies are apparent. Overall, the galaxy appears to be a relatively isolated system with a quiescent evolutionary state.
