The galaxy presents a generally smooth and elliptical morphology, with a subtle color gradient. The central region exhibits a slightly more concentrated luminosity, suggesting a bulge. The outer regions fade gradually, with no distinct spiral arm structures or prominent star-forming regions readily apparent. The overall color appears to be slightly redder suggesting an older stellar population. There is very minor evidence of disturbance in the morphology, possibly indicating a past or ongoing minor interaction. The galaxy appears to be relatively isolated in the field, showing no strong tidal features.
