The galaxy exhibits a generally elliptical morphology, appearing more elongated than circular. The light distribution suggests a smooth profile, with a high degree of central concentration. Its color is a gradient, with a central reddish hue transitioning to bluer tones in the outer regions, possibly indicative of varying stellar populations. The presence of these colors suggests the potential of ongoing or recent star formation, especially in the outer disk, or a composite stellar population with a mix of older and younger stars. There may be subtle disturbances in the overall structure, possibly indicating gravitational interactions with another galaxy, or internal dynamics.
