The galaxy presents as a somewhat smooth, elliptical structure with a moderate red color index, suggesting a dominant population of older stars. Its shape is neither perfectly round nor highly elongated, appearing somewhere in between. There is no significant evidence of a major ongoing merger or tidal disruption. Minor disturbances may be present, but the galaxy primarily exhibits a relaxed morphology. Based on its color and morphology, the galaxy is likely a relatively massive system with moderate levels of star formation.
