The galaxy presents as an elliptical or possibly lenticular morphology, appearing generally smooth in texture. It exhibits a bright, centrally concentrated core that fades gradually into a less luminous halo. There is a slight asymmetry to the overall light distribution, possibly indicating a minor gravitational disturbance or recent interaction. A faint, extended component or tidal feature may be present along one side of the galaxy. The color of the core is relatively blue, suggesting some ongoing star formation, though the overall stellar population is likely dominated by older, redder stars. There are no distinct spiral arms or dust lanes visible. The galaxy appears to be relatively isolated within its immediate environment.
