The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile, with the brightest region residing in the core. The overall shape approximates a sphere, showing high degree of roundness. There is no visible spiral arm structure or bar feature. The galaxy is slightly red in color, suggesting an older stellar population with reduced star formation activity. There is no evidence of a major ongoing merger or strong tidal disturbances, but a minor interaction cannot be ruled out.
