The galaxy presents as a smooth, elongated structure. Its morphology appears to be that of a spheroid, with a high degree of central concentration of light. The light distribution diminishes gradually from the core to the outer edges. A color gradient is present, transitioning from a relatively redder core to bluer outskirts. There are no discernible spiral arm features or dust lanes. Given the smooth appearance and color gradient, it could be an elliptical galaxy. The elongation implies a possible cigar shape morphology. There is no indication of any ongoing major merger activity or strong tidal disturbances in the immediate vicinity, however the smooth outer halo could indicate a potential minor disturbance from an earlier merger event.
