The galaxy presents as a largely smooth, elliptical structure with a centrally concentrated brightness profile. There is a radial color gradient, with a yellowish-white core transitioning to a redder outer halo. No distinct spiral arms or bar structures are apparent. The overall shape is nearly circular, lacking any significant elongation or tidal distortions, suggesting it is not currently undergoing a major merger event. Minor disturbances are not definitively excluded, but absent any clear indicators of tidal tails or asymmetric features, this appears to be a relatively relaxed system. The galaxy's red color implies an older stellar population with suppressed star formation activity, though this does not exclude a low level of residual star formation. The galaxy's moderate size indicates a substantial stellar mass.
