The galaxy presents as a moderately luminous, elliptical-shaped object. The overall color profile suggests a spectral energy distribution weighted toward the redder end of the visible spectrum, indicative of an older stellar population and/or significant dust obscuration. Its shape appears largely smooth, with a high degree of central concentration, and no obvious spiral arm structures or other prominent features. There might be a very faint, diffuse outer halo. The axis ratio suggests a classification leaning towards an E4 to E5 elliptical galaxy. It does not appear to be undergoing a major merger event, although some minor disturbances or tidal features cannot be entirely ruled out given the image resolution. Based on the apparent color and morphology, the galaxy is likely experiencing a relatively low rate of star formation.
