The galaxy appears as a smooth, elliptical structure with a concentrated central bulge. The light is dominated by yellow and red wavelengths, which suggests an older stellar population. The overall shape is fairly round, exhibiting minimal deviation from a spherical morphology. There is no distinct evidence of spiral arms, bars, or significant tidal disturbances. The galaxy exhibits a high degree of central concentration with a smooth transition to the outer regions. No indication of ongoing major mergers or significant star formation is visible.
